Theory of Star Formation

Abstract

We review current understanding of star formation, outlining an overall theoretical framework and the observations that motivate it. A conception of star formation has emerged in which turbulence plays a dual role, both creating overdensities to initiate gravitational contraction or collapse, and countering the effects of gravity in these overdense regions. The key dynamical processes involved in star formation -- turbulence, magnetic fields, and self-gravity -- are highly nonlinear and multidimensional. Physical arguments are used to identify and explain the features and scalings involved in star formation, and results from numerical simulations are used to quantify these effects. We divide star formation into large-scale and small-scale regimes and review each in turn. Large scales range from galaxies to giant molecular clouds (GMCs) and their substructures. Important problems include how GMCs form and evolve, what determines the star formation rate (SFR), and what determines the initial mass function (IMF). Small scales range from dense cores to the protostellar systems they beget. We discuss formation of both low- and high-mass stars, including ongoing accretion. The development of winds and outflows is increasingly well understood, as are the mechanisms governing angular momentum transport in disks. Although outstanding questions remain, the framework is now in place to build a comprehensive theory of star formation that will be tested by the next generation of telescopes.

120 pages, to appear in ARAA. No changes from v1 text; permission statement added

References in corpus (371)

• On the variation of the Initial Mass Function
• The Global Schmidt Law in Star Forming Galaxies
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The Milky Way in Molecular Clouds: A New Complete CO Survey
• Control of star formation by supersonic turbulence
• Disk Frequencies and Lifetimes in Young Clusters
• Spectral Energy Distributions of T Tauri Stars With Passive Circumstellar Disks
• Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
• SINGS: The SIRTF Nearby Galaxies Survey
• Toward Understanding Massive Star Formation
• Interstellar Turbulence I: Observations and Processes
• The Neutral Atomic Phases of the ISM in the Galaxy
• A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs
• The Stellar IMF from Turbulent Fragmentation
• The Formation of Massive Stars from Turbulent Cores
• Nonlinear Outcome of Gravitational Instability in Cooling, Gaseous Disks
• Cold Dark Clouds: The Initial Conditions for Star Formation
• The Star Formation Rate and Dense Molecular Gas in Galaxies
• The First Stars
• Using FU Orionis Outbursts to Constrain Self-Regulated Protostellar Disk Models
• Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting observed SEDs using a large grid of pre-computed models
• Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
• The Formation of a Star Cluster: Predicting the Properties of Stars and Brown Dwarfs
• The Relationship Between Gas Content and Star Formation in Molecule-Rich Spiral Galaxies
• Accretion Disks around Young Objects. I. The Detailed Vertical Structure
• The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
• Slow Star Formation in Dense Gas: Evidence and Implications
• Dense Cores in Dark Clouds. XIV. N2H+(1-0) maps of dense cloud cores
• Star formation thresholds and galaxy edges: why and where
• Competitive accretion in embedded stellar cluster
• The Formation of Brown Dwarfs as Ejected Stellar Embryos
• The Anisotropy of MHD Alfvénic Turbulence
• On the Formation of Massive Stars
• Dynamical Friction in a Gaseous Medium
• The Millennium Arecibo 21-CM Absorption Line Survey. II. Properties of the Warm and Cold Neutral Media
• Very Low Mass Stars and Brown Dwarfs in Taurus-Auriga
• Simulations of Incompressible MHD Turbulence
• Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
• Compressible Magnetohydrodynamic Turbulence: mode coupling, scaling relations, anisotropy, new regime and astrophysical implications
• Star Formation in a Crossing Time
• Dissipation in Compressible MHD Turbulence
• Observational Constraints on the Formation and Evolution of Binary Stars
• The Energy Dissipation Rate of Supersonic, Magnetohydrodynamic Turbulence in Molecular Clouds
• Kinetic Energy Decay Rates of Supersonic and Super-Alfvenic Turbulence in Star-Forming Clouds
• The Universality of Turbulence in Galactic Molecular Clouds
• Star Formation Thresholds in Galactic Disks
• Photoevaporation of protoplanetary discs II: evolutionary models and observable properties
• The mass function of dense molecular cores and the origin of the IMF
• Observations of IC348: The Disk Population at 2-3 Million Years
• Photoevaporation of Circumstellar Disks due to External FUV Radiation in Stellar Aggregates
• The Formation of a Bound Star Cluster: From the Orion Nebula Cluster to the Pleiades
• Massive molecular outflows
• On the formation of massive stars
• The effect of dust settling on the appearance of protoplanetary disks
• Can giant planets form by direct gravitational instability?
• The hierarchical formation of a stellar cluster
• Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions
• Enhanced Angular Momentum Transport in Accretion Disks
• High Resolution Submillimeter Constraints on Circumstellar Disk Structure
• Accretion in Young Stellar/Substellar Objects
• Effects of Dust Growth and Settling in T Tauri Disks
• Simulations of MHD Turbulence in a Strongly Magnetized Medium
• Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
• Magnetic Fields in the Formation of Sun-Like Stars
• Star formation through gravitational collapse and competitive accretion
• Efficiencies of Low-Mass Star and Star Cluster Formation
• A Super-Alfvenic Model of Dark Clouds
• The Burst Mode of Protostellar Accretion
• Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
• The Mass Function of Young Star Clusters in the "Antennae" Galaxies
• Molecular Cloud Evolution II. From cloud formation to the early stages of star formation in decaying conditions
• The Physics of Star Formation
• The locality of transport in self-gravitating accretion discs
• Density probability distribution in one-dimensional polytropic gas dynamics
• Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation
• On the Evolutionary Status of Class I Stars and Herbig-Haro Energy Sources in Taurus-Auriga
• Investigating fragmentation conditions in self-gravitating accretion discs
• Simulations of nonhelical hydromagnetic turbulence
• Star formation in clusters: a survey of compact mm-wave sources in the Serpens core
• Enhanced cosmic-ray flux toward zeta Persei inferred from laboratory study of H3+ - e- recombination rate
• The initial mass function : from Salpeter 1955 to 2005
• Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. I. Perseus
• Episodic accretion in magnetically layered protoplanetary discs
• Helical Fields and Filamentary Molecular Clouds
• Star Formation from Galaxies to Globules
• Interstellar Turbulence II: Implications and Effects
• Stellar Multiplicity and the IMF: Most Stars Are Single
• On the Role of Massive Stars in the Support and Destruction of Giant Molecular Clouds
• An upper limit to the masses of stars
• Feedback, Disk Self-regulation and Galaxy Formation
• The Equilibrium State of Molecular Regions in the Outer Galaxy
• The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
• Turbulent Flow-Driven Molecular Cloud Formation: A Solution to the Post-T Tauri Problem?
• The Evolution of Outflow-Envelope Interactions in Low-Mass Protostars
• Angular Momentum Transport by MHD Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability
• One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-Gravitating Media
• Star formation in Perseus - V. Outflows detected by HARP
• A study of high velocity molecular outflows with an up-to-date sample
• The Origin of Episodic Accretion Bursts in the Early Stages of Star Formation
• Photoevaporation of protoplanetary discs I: hydrodynamic models
• Collapse of Magnetized Singular Isothermal Toroids: II. Rotation and Magnetic Braking
• The "Mysterious" Origin of Brown Dwarfs
• Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions
• The Millennium Arecibo 21-cm Absorption Line Survey. IV. Statistics of Magnetic Field, Column Density, and Turbulence
• The COMPLETE Survey of Star-Forming Regions: Phase I Data
• Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks
• HST/STIS Spectroscopy of the Optical Outflow from DG Tau: Indications for Rotation in the Initial Jet Channel
• The ionization fraction in alpha-models of protoplanetary disks
• Measuring Accretion in Young Substellar Objects: Approaching the Planetary Mass Regime
• The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation
• Dense Gas and Star Formation: Characteristics of Cloud Cores Associated with Water Masers
• Bolocam Survey for 1.1 mm Dust Continuum Emission in the c2d Legacy Clouds. II. Ophiuchus
• On the Origin of the Global Schmidt Law of Star Formation
• Photoevaporation of Circumstellar Disks around Young Stars
• On the mass function of star clusters
• Outflows and Jets from Collapsing Magnetized Cloud Cores
• Accretion in stellar clusters and the IMF
• Molecular cloud evolution. I. Molecular cloud and thin CNM sheet formation
• The Star Formation Rate in disk galaxies: thresholds and dependence on gas amount
• Large dust particles in disks around T Tauri stars
• Global Star Formation Rates in Disk Galaxies and Circumnuclear Starbursts from Cloud Collisions
• Discovery of Recent Star Formation in the Extreme Outer Regions of Disk Galaxies
• Clouds as Turbulent Density Fluctuations. Implications for pressure confinement and spectral line data interpretation
• 2MASS wide field extinction maps - I. The Pipe nebula
• HST/STIS spectroscopy of the optical outflow from DG Tau: structure and kinematics on sub-arcsecond scales
• Equilibrium Star Cluster Formation
• The initial conditions of isolated star formation - VI. SCUBA mapping of prestellar cores
• Spectral energy dynamics in magnetohydrodynamic turbulence
• The Birth of High Mass Stars: Accretion and/or Mergers?
• Differential Rotation and Turbulence in Extended HI Disks
• The Large and Small Scale Structures of Dust in the Star-Forming Perseus Molecular Cloud
• The Role of Pressure in GMC Formation
• On the Density Probability Function of Galactic Gas. I. Numerical Simulations and the Significance of the Polytropic Index
• Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
• The Formation of Massive Stars by Accretion Through Trapped Hypercompact HII Regions
• Supersonic turbulence in the ISM: stellar extinction determinations as probes of the structure and dynamics of dark clouds
• A SCUBA survey of Orion, the low-mass end of the core mass function
• A Survey for Infall Motions toward Starless Cores. I. CS (2-1) and N${}_2$H${}^{+}$ (1-0) Observations
• Kinetic and Structural Evolution of Self-gravitating, Magnetized Clouds: 2.5-Dimensional Simulations of Decaying Turbulence
• Giant Molecular Clouds in M33 -- II. High Resolution Observations
• Molecular Cloud Formation Behind Shock Waves
• Mechanism of Magnetic Flux Loss in Molecular Clouds
• The evolution of gravitationally unstable protoplanetary disks: fragmentation and possible giant planet formation
• Turbulent Mixing and the Dead Zone in Protostellar Disks
• Collapse of Rotating Magnetized Molecular Cloud Cores and Mass Outflows
• Cluster Formation in Protostellar Outflow-Driven Turbulence
• The Global Evolution of Giant Molecular Clouds. I: Model Formulation and Quasi-Equilibrium Behavior
• Effects of the Equation of State on the Formation of Star Clusters
• The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State
• The Mass Spectra of Giant Molecular Clouds in the Local Group
• Photoionising feedback in star cluster formation
• A dynamical origin for early mass segregation in young star clusters
• The thermodynamics of collapsing molecular cloud cores using smoothed particle hydrodynamics with radiative transfer
• An Extinction Threshold for Protostellar Cores in Ophiuchus
• Formation of Structure in Molecular Clouds: A Case Study
• Fragmentation of Massive Protostellar Disks
• IRAS 05358+3543: Multiple outflows at the earliest stages of massive star formation
• The Effect of the Hall Term on the Nonlinear Evolution of the Magnetorotational Instability: II. Saturation Level and Critical Magnetic Reynolds Number
• Physical vs. Observational Properties of Clouds in Turbulent Molecular Cloud Models
• The Formation of Free-Floating Brown Dwarves and Planetary-Mass Objects by Photo-Erosion of Prestellar Cores
• Nonlinear Outcome of Gravitational Instability in Disks with Realistic Cooling
• The Molecular Gas Distribution and Schmidt Law in M33
• New Protostellar Collapse Candidates: An HCO+ Survey of the Class 0 Sources
• A SCUBA survey of the NGC 2068/2071 protoclusters
• A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
• Formation of massive stars by growing accretion rate
• Formation and Fragmentation of Gaseous Spurs in Spiral Galaxies
• Statistical anisotropy of magnetohydrodynamic turbulence
• The Thermal Regulation of Gravitational Instabilities in Protoplanetary Disks III. Simulations with Radiative Cooling and Realistic Opacities
• Locating the Launching Region of T Tauri Winds: The Case of DG Tau
• The Lifetimes and Evolution of Molecular Cloud Cores
• Local Hydrodynamic Stability of Accretion Disks
• Towards Planetesimals in the Disk around TW Hya: 3.5 centimeter Dust Emission
• Protostellar Disks: Formation, Fragmentation, and the Brown Dwarf Desert
• Why Do T Tauri Disks Accrete?
• High-Resolution Spectroscopy in Tr37: Gas Accretion Evolution in Evolved Dusty Disks
• The Thermal Regulation of Gravitational Instabilities in Protoplanetary Disks II. Extended Simulations with Varied Cooling Rates
• The Formation of Self-Gravitating Cores in Turbulent Magnetized Clouds
• The Formation of Stellar Clusters: Gaussian Initial Conditions II
• Gravitational collapse of magnetized clouds. I. Ideal MHD accretion flow
• Gravitational Collapse and Star Formation in Logotropic and Non-Isothermal Spheres
• Near Infrared Imaging Survey of Bok Globules: Density Structure
• New OH Zeeman measurements of magnetic field strengths in molecular clouds
• Velocity Modification of Power Spectrum from Absorbing Medium
• Turbulent Molecular Cloud Cores: Rotational Properties
• Statistical Confirmation of a Stellar Upper Mass Limit
• HI Narrow Self-Absorption in Dark Clouds: Correlations with Molecular Gas and Implications for Cloud Evolution and Star Formation
• Hydrodynamical Simulations of Jet- and Wind-driven Protostellar Outflows
• An unbiased search for the signatures of protostars in the rho Ophiuchi Molecular Cloud. II. Millimetre continuum observations
• Three-Dimensional Vortices in Stratified Protoplanetary Disks
• Binary systems and stellar mergers in massive star formation
• Collapse-Driven Outflow in Star-Forming Molecular Cores
• Formation of Spiral-Arm Spurs and Bound Clouds in Vertically Stratified Galactic Gas Disks
• Amplification, Saturation, and Q Thresholds for Runaway: Growth of Self-Gravitating Structures in Models of Magnetized Galactic Gas Disks
• Kolmogorov-Burgers Model for Star Forming Turbulence
• Quiescent and coherent cores from gravoturbulent fragmentation
• A Uniform CO Survey of the Molecular Clouds in Orion and Monoceros
• Supersonic Turbulence and the Fragmentation of a Cold Medium
• A complete 12CO 2-1 map of M51 with HERA: I. Radial averages of CO, HI, and radio continuum
• Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?
• Scaling relations of supersonic turbulence in star-forming molecular clouds
• Probing the inner 200 AU of low-mass protostars with the Submillimeter Array: Dust and organic molecules in NGC1333-IRAS2A
• How Protostellar Outflows Help Massive Stars Form
• Accretion Disks around Young Stars: Lifetimes, Disk Locking and Variability
• Limits on the primordial stellar multiplicity
• The Physical Natures of Class I and Flat-Spectrum Protostellar Photospheres: A Near-Infrared Spectroscopic Study
• Recipes for stellar jets: results of combined optical/infrared diagnostics
• Observations on the Formation of Massive Stars by Accretion
• Infall Collapse Solutions in the Inner Limit: Radiation Pressure and its Effects on Star Formation
• Three-Dimensional Simulations of Parker, Magneto-Jeans, and Swing Instabilities in Shearing Galactic Gas Disks
• Dynamical HII Region Evolution in Turbulent Molecular Clouds
• Dynamical Evidence for a Luminous, Young Globular Cluster in NGC 1569
• Global Modeling of Spur Formation in Spiral Galaxies
• Six Myths on the Virial Theorem for Interstellar Clouds
• The Vertical Distribution and Kinematics of HI and Mass Models of the Galactic Disk
• Quiescent Cores and the Efficiency of Turbulence-Accelerated, Magnetically Regulated Star Formation
• The secrets of the nearest starburst cluster: II. The present-day mass function in NGC 3603
• The Probability Distribution Function of Column Density in Molecular Clouds
• Density Power Spectrum of Compressible Hydrodynamic Turbulent Flows
• A Search for Larson-Type Relations in Numerical Simulations of the ISM. Evidence for Non-Constant Column Densities
• Analysis of Clumps in Molecular Cloud Models: Mass Spectrum, Shapes, Alignment and Rotation
• Consistency of Ambipolar Diffusion Models with Infall in the L1544 Protostellar Core
• High Mass Starless Cores
• Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results
• The initial stellar mass function from random sampling in hierarchical clouds II: statistical fluctuations and a mass dependence for starbirth positions and times
• Ambipolar-Diffusion Timescale, Star-Formation Timescale, and the Ages of Molecular Clouds: Is There a Discrepancy?
• A Model for the Internal Structure of Molecular Cloud Cores
• Magnetorotationally-Driven Galactic Turbulence and the Formation of Giant Molecular Clouds
• Radiation Feedback and Fragmentation in Massive Protostellar Cores
• The Virial Balance of Clumps and Cores in Molecular Clouds
• N2H+(1-0) survey of massive molecular cloud cores
• Simulating Star Formation and Feedback in Galactic Disk Models
• Binary stars in young clusters: models versus observations of the Trapezium Cluster
• The Jeans mass and the origin of the knee in the IMF
• Bipolar molecular outflows driven by hydromagnetic protostellar winds
• Spectral Properties of Compressible Magnetohydrodynamic Turbulence from Numerical Simulations
• Star formation in unbound giant molecular clouds: the origin of OB associations?
• The Power Spectrum of Supersonic Turbulence in Perseus
• Magnetic Fields and the Triaxiality of Molecular Cloud Cores
• Magnetic Fields in Diffuse H I and Molecular Clouds
• Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse
• Magnetically Dominated Strands of Cold Hydrogen in the Riegel-Crutcher Cloud
• Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
• Magnetohydrodynamic Instabilities in Shearing, Rotating, Stratified Winds and Disks
• Investigating grain growth in disks around southern T Tauri stars at millimetre wavelengths
• Ambipolar Drift in a Turbulent Medium
• New Regime of MHD Turbulence: Cascade Below Viscous Cutoff
• Self-similar Collapse of Rotating Magnetic Molecular Cloud Cores
• Bypass to Turbulence in Hydrodynamic Accretion: Lagrangian Analysis of Energy Growth
• The Spectral Correlation Function -- A New Tool for Analyzing Spectral-Line Maps
• Protostellar outflow-driven turbulence
• A New High Resolution CO Map of the inner 2.'5 of M51 I. Streaming Motions and Spiral Structure
• The Stellar Initial Mass Function
• Magnetorotational instability in protoplanetary discs
• Structure Function Scaling in Compressible Super-Alfvenic MHD Turbulence
• Turbulence driven by outflow-blown cavities in the molecular cloud of NGC 1333
• Star Formation at High Angular Resolution
• High Mass Star Formation I: The Mass Distribution of Submillimeter Clumps in NGC 7538
• Bondi-Hoyle Accretion in a Turbulent Medium
• Does Magnetic Levitation or Suspension Define the Masses of Forming Stars?
• HH 212: SMA Observations of a Remarkable Protostellar Jet
• An HST Archival Survey of Feathers in Spiral Galaxies
• On hydrodynamic shear turbulence in Keplerian disks: via transient growth to bypass transition
• Control of Star Formation in Galaxies by Gravitational Instability
• The Shapes of Dense Cores and Bok Globules
• The Formation of Star Clusters I: 3D Simulations of Hydrodynamic Turbulence
• Molecular gas in the galaxy M83. I - The molecular gas distribution
• The Global Baroclinic Instability in Accretion Disks. II: Local Linear Analysis
• Cloudshine: New Light on Dark Clouds
• A Turbulent Interstellar Medium Origin of the Binary Period Distribution
• A Solution to the Protostellar Accretion Problem
• On the dynamics of magnetorotational turbulent stresses
• Collimation of astrophysical jets - the role of the accretion disk magnetic field distribution
• Turbulent Cooling Flows in Molecular Clouds
• Modeling a high mass turn down in the stellar initial mass function
• Vortices in Thin, Compressible, Unmagnetized Disks
• Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
• Enhancement of Ambipolar Diffusion Rates through Field Fluctuations
• Super-Sonic Turbulence in the Perseus Molecular Cloud
• Self-Similar Magnetocentrifugal Disk Winds with Cylindrical Asymptotics
• Caught in the act: The Onset of massive star formation
• The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
• Spherical Infall in G10.6-0.4: Accretion Through an Ultracompact HII Region
• Star Formation in Space and Time: The Orion Nebula Cluster
• Fragmentation in Massive Star Formation
• Three Dimensional Compressible Hydrodynamic Simulations of Vortices in Disks
• Gravitational Runaway and Turbulence Driving in Star-Gas Galactic Disks
• Intrinsic Shapes of Molecular Cloud Cores
• Turbulent Ambipolar Diffusion: Numerical Studies in 2D
• Centrally condensed turbulent cores: Massive stars or fragmentation?
• Massive Field Stars and the Stellar Clustering Law
• Very compact radio emission from high-mass protostars. II. Dust disks and ionized accretion flows
• Turbulent Gas Flows in the Rosette and G216-2.5 Molecular Clouds: Assessing Turbulent Fragmentation Descriptions of Star Formation
• Controlling the collimation and rotation of hydromagnetic disk winds
• Multifractal Scaling, Geometrical Diversity, and Hierarchical Structure in the Cool Interstellar Medium
• Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
• Precursors of UCHII regions & the evolution of massive outflows
• The Structure of Magnetocentrifugal Winds I. Steady Mass Loading
• Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
• Magneto-Centrifugal Launching of Jets from Accretion Disks. II: Inner Disk-Driven Winds
• Linear Theory of Thin, Radially-Stratified Disks
• Protostellar mass accretion rates from gravoturbulent fragmentation
• Formation and loss of hierarchical structure in two-dimensional MHD simulations of wave-driven turbulence in interstellar clouds
• Magnetically Controlled Spasmodic Accretion During Star Formation. II. Results
• Dynamical Collapse of Nonrotating Magnetic Molecular Cloud Cores: Evolution Through Point-Mass Formation
• An Upper Limit on the Mass of a Primordial Star due to the Formation of an HII Region: The Effect of Ionizing Radiation Force
• IRAC and MIPS Observations of the Interacting Galaxies IC 2163 and NGC 2207: Clumpy Emission
• Generalized Collapse Solutions with Nonzero Initial Velocities for Star Formation in Molecular Cloud Cores
• Multi--Pressure Polytropes as Models for the Structure and Stability of Molecular Clouds. I. Theory
• Molecular gas in NGC6946
• Dark cloud cores and gravitational decoupling from turbulent flows
• The Inability of Ambipolar Diffusion to set a Characteristic Mass Scale in Molecular Clouds
• Adaptive Mesh Refinement for Supersonic Molecular Cloud Turbulence
• Does Infall End Before the Class I Stage?
• A ballistic bow shock model for jet-driven protostellar outflow shells
• The Star Formation Threshold in NGC 6822
• High Mass Star Formation. II. The Mass Function of Submillimeter Clumps in M17
• Brown dwarf formation by binary disruption
• The effect of a finite mass reservoir on the collapse of spherical isothermal clouds and the evolution of protostellar accretion
• Centrally Condensed Collapse of Starless Cores
• Collapse of Magnetized Singular Isothermal Toroids: I. Non-Rotating Case
• The Schmidt Law at High Molecular Densities
• The Intrinsic Shapes of Molecular Cloud Fragments over a Range of Length Scales
• The Three-Dimensional Structure of a Massive Gas Disk in the Galactic Central Region
• Radio continuum and CO emission in star-forming galaxies
• High Mass Star Formation. III. The Functional Form of the Submillimeter Clump Mass Function
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: II. Typical Axisymmetric Solution
• Protostellar Angular Momentum Evolution during Gravoturbulent Fragmentation
• From Dusty Filaments to Cores to Stars: An Infrared Extinction Study of Lupus 3
• Stellar Mass Spectra from Non-Isothermal Gravoturbulent Fragmentation
• Oscillations of starless cores
• Does Turbulent Pressure Behave as a Logatrope?
• Interaction of Infall and Winds in Young Stellar Objects
• Composite Polytrope Models of Molecular Clouds. I. Theory
• Interstellar Turbulence Driving by Galactic Spiral Shocks
• Far-Infrared Spectral Energy Distributions of Embedded Protostars and Dusty Galaxies: I. Theory for Spherical Sources
• Giant Molecular Clouds are More Concentrated to Spiral Arms than Smaller Clouds
• The Eastern Arm of M83 Revisited: High-Resolution Mapping of 12CO 1-0 Emission
• On the Effects of Projection on Morphology
• Self-Similar Collapse of Nonrotating Magnetic Molecular Cloud Cores
• Hubble Space Telescope NICMOS Imaging of W3 IRS 5: A Trapezium in the Making?
• Three-Dimensional Evolution of the Parker Instability under a Uniform Gravity
• The Effect of Radiative Feedback on Bondi--Hoyle Flow around a Massive Star
• Looking for Distributed Star Formation in L1630: A Near-infrared (J, H, K) Survey
• The Initial Conditions for Gravitational Collapse of a Core: An Extremely Young Low-Mass Class 0 Protostar GF9-2
• Three-dimensional Simulations of the Parker Instability in a Uniformly-rotating Disk
• Can WNM survive inside Molecular Clouds ?
• Outflow Driven Cavities: Numerical Simulations of Intermediaries of Protostellar Turbulence
• Interstellar cloud structure: The statistics of centroid velocities
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: I. Formulation of the Problem and Method of Solution
• Nonlinear Stability of Thin, Radially-Stratified Disks
• Dynamics and Structure of Three-Dimensional Trans-Alfvenic Jets. II. The Effect of Density and Winds
• High Resolution Mapping of Interstellar Clouds by Near--IR Scattering
• Toward Resolving the Outflow Engine: An Observational Perspective
• A New Algorithm for Radiative Feedback and its Application to the Formation of Massive Stars
• Magnetocentrifugal Winds in 3D: Nonaxisymmetric Steady State
• The Parker Instability in a Thick Gaseous Disk II: Numerical Simulations in 2D
• Wave Motions In Molecular Clouds: Results in Two Dimensions
• Astrochemical confirmation of the rapid evolution of massive YSOs and explanation for the inferred ages of hot cores
• Stellar Outflows Driven by Magnetized Wide-Angle Winds
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: III. A Parameter Study
• Electron Abundance in Protostellar Cores
• Massive Star Outflows
• Radiation Pressure in Massive Star Formation
• The distribution of ejected brown dwarfs in clusters
• A review of the theory of incompressible MHD turbulence
• Nonlinear Criterion for the Stability of Molecular Clouds
• The chemistry of high-mass star formation
• On the transfer of momentum from stellar jets to molecular outflows
• 2-D and 3-D Radiation Transfer Models of High-Mass Star Formation

Cited by in corpus (1629)

• Star Formation in the Milky Way and Nearby Galaxies
• The CO-to-H2 Conversion Factor
• Simulating Galaxy Formation with the IllustrisTNG Model
• The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
• The Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Physical Models of Galaxy Formation in a Cosmological Framework
• Stellar Multiplicity
• Toward Understanding Massive Star Formation
• The Galactic Center Massive Black Hole and Nuclear Star Cluster
• The SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies
• Cold Dark Clouds: The Initial Conditions for Star Formation
• A Universal Stellar Initial Mass Function? A Critical Look at Variations
• A Study of the Gas-Star Formation Relation over Cosmic Time
• PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies
• Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
• Dusty Star-Forming Galaxies at High Redshift
• Multiple populations in globular clusters. Lessons learned from the Milky Way globular clusters
• Characterizing interstellar filaments with Herschel in IC5146
• The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
• Different star formation laws for disks versus starbursts at low and high redshifts
• The Dark Molecular Gas
• ATLASGAL - The APEX Telescope Large Area Survey of the Galaxy at 870 microns
• Star Clusters Across Cosmic Time
• Re-examining Larson's Scaling Relationships in Galactic Molecular Clouds
• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
• Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass
• The rotation rates of massive stars: the role of binary interaction through tides, mass transfer and mergers
• What Drives the Growth of Black Holes?
• A Universal, Local Star Formation Law in Galactic Clouds, Nearby Galaxies, High-Redshift Disks, and Starbursts
• The Resolved Properties of Extragalactic Giant Molecular Clouds
• The First Galaxies
• Towards a complete accounting of energy and momentum from stellar feedback in galaxy formation simulations
• Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars
• The Disruption of Giant Molecular Clouds by Radiation Pressure and the Efficiency of Star Formation in Galaxies
• The Birth Environment of the Solar System
• The Atomic to Molecular Transition in Galaxies. II: HI and H_2 Column Densities
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types
• Probing the evolution of molecular cloud structure: From quiescence to birth
• On the fraction of star formation occurring in bound stellar clusters
• Evolution of Massive Protostars with High Accretion Rates
• Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
• A Constant Molecular Gas Depletion Time in Nearby Disk Galaxies
• Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH
• Regulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/Dynamical Equilibrium Model
• Momentum Injection by Supernovae in the Interstellar Medium
• On the Star Formation Efficiency of Turbulent Magnetized Clouds
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
• Unresolved stellar companions with Gaia DR2 astrometry
• Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps
• Extrasolar planet population synthesis IV. Correlations with disk metallicity, mass and lifetime
• Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario
• Numerical Tests of Fast Reconnection in Weakly Stochastic Magnetic Fields
• Dynamic star formation in the massive DR21 filament
• Turbulent molecular clouds
• Escape fraction of ionizing photons during reionization: effects due to supernova feedback and runaway OB stars
• The formation of the first stars and galaxies
• Formation of the First Stars
• Galaxy Formation Theory
• Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
• Chaotic star formation and the alignment of stellar rotation with disc and planetary orbital axes
• The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks
• The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function
• Chemistry of Dark Clouds: Databases, Networks, and Models
• PS1-10jh: The Disruption of a Main-Sequence Star of Near-Solar Composition
• Molecular Hydrogen and Global Star Formation Relations in Galaxies
• The first stars: formation of binaries and small multiple systems
• Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
• Low Virial Parameters in Molecular Clouds: Implications for High Mass Star Formation and Magnetic Fields
• A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence
• On the universality of supersonic turbulence
• The Structure of the Interstellar Medium of Star Forming Galaxies
• Identifying the Low Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
• The metallicity dependence of the CO {\rightarrow} H_2 conversion factor in z>1 star forming galaxies
• The Bolocam Galactic Plane Survey: Survey Description and Data Reduction
• Galaxy alignments: An overview
• The formation of disc galaxies in a LCDM universe
• Star Formation in Disk Galaxies. I. Formation and Evolution of Giant Molecular Clouds via Gravitational Instability and Cloud Collisions
• ATLASGAL - Compact source catalogue: 330 < l < 21 degrees
• Circumventing the radiation pressure barrier in the formation of massive stars via disk accretion
• The PdBI Arcsecond Whirlpool Survey (PAWS): Environmental Dependence of Giant Molecular Cloud Properties in M51
• The PHANGS-MUSE survey -- Probing the chemo-dynamical evolution of disc galaxies
• An Imprint of Molecular Cloud Magnetization in the Morphology of the Dust Polarized Emission
• Inefficient star formation through turbulence, magnetic fields and feedback
• Modeling Molecular Hydrogen and Star Formation in Cosmological Simulations
• Astrochemistry and compositions of planetary systems
• Gravity or Turbulence? The velocity dispersion-size relation
• Cosmic evolution of the atomic and molecular gas content of galaxies
• Extending Big Power Law in the Sky with Turbulence Spectra from WHAM data
• Three-phase Interstellar medium in Galaxies Resolving Evolution with Star formation and Supernova feedback (TIGRESS): Algorithms, Fiducial model, and Convergence
• Recent progress in astrophysical plasma turbulence from solar wind observations
• Modeling UV Radiation Feedback from Massive Stars: II. Dispersal of Star-Forming Giant Molecular Clouds by Photoionization and Radiation Pressure
• Evidence of Cosmic Evolution of the Stellar Initial Mass Function
• The dynamical evolution of molecular clouds near the Galactic Centre - I. Orbital structure and evolutionary timeline
• The propagation of uncertainties in stellar population synthesis modeling II: The challenge of comparing galaxy evolution models to observations
• The Westerbork SINGS Survey II. Polarization, Faraday Rotation, and Magnetic Fields
• Clump morphology and evolution in MHD simulations of molecular cloud formation
• Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus
• Formation of Massive Molecular Cloud Cores by Cloud-cloud Collision
• Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas
• Environmental Dependence of the Kennicutt-Schmidt Relation in Galaxies
• The mass function of young star clusters in spiral galaxies
• The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic Cloud
• Systematic variation of the stellar Initial Mass Function with velocity dispersion in early-type galaxies
• Stellar Feedback in Molecular Clouds and its Influence on the Mass Function of Young Star Clusters
• Magnetic Fields in High-Mass Infrared Dark Clouds
• Evolution of Spin Direction of Accreting Magnetic Protostars and Spin-Orbit Misalignment in Exoplanetary Systems
• The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016
• The Ubiquity of Micrometer-Sized Dust Grains in the Dense Interstellar Medium
• Magnetically Regulated Star Formation in 3D: The Case of Taurus Molecular Cloud Complex
• 3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications
• On the universality of interstellar filaments: theory meets simulations and observations
• Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum
• Hall-effect Controlled Gas Dynamics in Protoplanetary Disks: II. Full 3D Simulations toward the Outer Disk
• Limiting Accretion onto Massive Stars by Fragmentation-Induced Starvation
• Evolution of the atomic and molecular gas content of galaxies
• Cooling, Gravity and Geometry: Flow-driven Massive Core Formation
• Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters II. The Initial Mass Function from Winds, Turbulence, and Radiation
• Modeling CO Emission: I. CO as a Column Density Tracer and the X-Factor in Molecular Clouds
• Gas Kinematics on GMC scales in M51 with PAWS: cloud stabilization through dynamical pressure
• A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey
• STARFORGE: Toward a comprehensive numerical model of star cluster formation and feedback
• Modeling jet and outflow feedback during star cluster formation
• The properties of the ISM in disc galaxies with stellar feedback
• The Plateau de Bure + 30m Arcsecond Whirlpool Survey reveals a thick disk of diffuse molecular gas in the M51 galaxy
• Partially Ionized Plasmas in Astrophysics
• MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey
• Velocity Field of Compressible MHD Turbulence: Wavelet Decomposition and Mode Scalings
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• The Stellar IMF, Core Mass Function, & The Last-Crossing Distribution
• The Long-term Evolution of the Galactic Disk Traced by Dissolving Star Clusters
• A robust numerical scheme for highly compressible magnetohydrodynamics: Nonlinear stability, implementation and tests
• Accretion disks in luminous young stellar objects
• The Birth of a Galaxy. II. The Role of Radiation Pressure
• The Origin of Massive Stars: The Inertial-Inflow Model
• Variations in the Star Formation Efficiency of the Dense Molecular Gas across the Disks of Star-Forming Galaxies
• The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim 2.6$ to $z\sim 0.6$ with KMOS${}^{3D}$
• Ages and Luminosities of Young SMC/LMC Star Clusters and the recent Star Formation History of the Clouds
• Jeans analysis of self-gravitating systems in f(R)-gravity
• Modelling CO formation in the turbulent interstellar medium
• Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model
• The dynamical state of stellar structure in star-forming regions
• Unifying low and high mass star formation through density amplified hubs of filaments
• The CO-H2 Conversion Factor in Disc Galaxies and Mergers
• Tidal Truncation of Inclined Circumstellar and Circumbinary Discs in Young Stellar Binaries
• On the impact of empirical and theoretical star formation laws on galaxy formation
• On the evolution of the density pdf in strongly self-gravitating systems
• Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
• SMA Observations of Class 0 Protostars: A High-Angular Resolution Survey of Protostellar Binary Systems
• The Star Formation Law in Molecule-Poor Galaxies
• Galactic cold cores III. General cloud properties
• Radiation-magnetohydrodynamic simulations of HII regions and their associated PDRs in turbulent molecular clouds
• Compressible Turbulence: The Cascade and its Locality
• The formation and hierarchical assembly of globular cluster populations
• High-dynamic-range extinction mapping of infrared dark clouds: Dependence of density variance with sonic Mach number in molecular clouds
• The Physical Nature of Starburst-Driven Galactic Outflows
• Molecular Cloud Evolution IV: Magnetic Fields, Ambipolar Diffusion, and the Star Formation Efficiency
• A hot compact dust disk around a massive young stellar object
• Modeling CO Emission: II. The Physical Characteristics that Determine the X factor in Galactic Molecular Clouds
• Wave-like warp propagation in circumbinary discs I. Analytic theory and numerical simulations
• The Mass-Size Relation from Clouds to Cores. II. Solar Neighborhood Clouds
• Neutrino-dominated accretion flows as the central engine of gamma-ray bursts
• Rapid Molecular Cloud and Star Formation: Mechanisms and Movies
• Cloud Scale ISM Structure and Star Formation in M51
• Magnetic field amplification in turbulent astrophysical plasmas
• The sonic scale revealed by the world's largest supersonic turbulence simulation
• A Model for the Origin of Bursty Star Formation in Galaxies
• On the dust temperatures of high redshift galaxies
• The interplay between a galactic bar and a supermassive black hole: nuclear fueling in a sub-parsec resolution galaxy simulation
• Magnetic fields during the early stages of massive star formation - I. Accretion and disk evolution
• What determines the grain size distribution in galaxies?
• An all-sky Support Vector Machine selection of WISE YSO Candidates
• Shattering and coagulation of dust grains in interstellar turbulence
• GMC formation by agglomeration and self gravity
• Star cluster formation in cosmological simulations. I. Properties of young clusters
• Characterizing Magnetohydrodynamic Turbulence in the Small Magellanic Cloud
• Radiation-Hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows
• Molecular Rings and the Thickness of Star-Forming Clouds
• Constraining the Time Interval for the Origin of Life on Earth
• A simple and accurate approximation for the Q stability parameter in multi-component and realistically thick discs
• The Small-Scale Dynamo and Non-Ideal MHD in Primordial Star Formation
• Cloud-cloud collisions and triggered star formation
• The Star Formation Efficiency per Free Fall Time in Nearby Galaxies
• The Link between Magnetic Fields and Filamentary Clouds: Bimodal Cloud Orientations in the Gould Belt
• Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
• The linewidth-size relationship in the dense ISM of the Central Molecular Zone
• The Dawes Review 8: Measuring the Stellar Initial Mass Function
• How long does it take to form a molecular cloud?
• Turbulence-induced magnetic fields and the structure of Cosmic Ray modified shocks
• The PHANGS-HST Survey: Physics at High Angular resolution in Nearby GalaxieS with the Hubble Space Telescope
• Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters I. Implications for the Origin of the Initial Mass Function
• The Global Evolution of Giant Molecular Clouds II: The Role of Accretion
• The Protostellar Luminosity Function
• The Formation and Gravitational-Wave Detection of Massive Stellar Black-Hole Binaries
• Growth of Magnetic Fields Induced by Turbulent Motions
• SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium
• Testing Magnetic Star Formation Theory
• The Star Formation Rate in the Gravoturbulent Interstellar Medium
• Star Cluster Formation in Turbulent, Magnetized Dense Clumps with Radiative and Outflow Feedback
• A Godunov Method for Multidimensional Radiation Magnetohydrodynamics based on a variable Eddington tensor
• Complex Structure in Class 0 Protostellar Envelopes II: Kinematic Structure from Single-Dish and Interferometric Molecular Line Mapping
• First hydrodynamics simulations of radiation forces and photoionization feedback in massive star formation
• The Turbulent Origin of Spin-Orbit Misalignment in Planetary Systems
• Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
• The Super-linear Slope of the Spatially-Resolved Star Formation Law in NGC 3521 and NGC 5194 (M51a)
• The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$
• Turbulence, Magnetic Reconnection in Turbulent Fluids and Energetic Particle Acceleration
• Superdiffusion of Cosmic Rays: Implications for Cosmic Ray Acceleration
• Velocity Gradients as a Tracer for Magnetic Fields
• The efficiency of star formation in clustered and distributed regions
• Tracing magnetic fields with spectroscopic channel maps
• Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
• Vertical Equilibrium, Energetics, and Star Formation Rates in Magnetized Galactic Disks Regulated by Momentum Feedback from Supernovae
• Gas dynamics in Massive Dense Cores in Cygnus-X
• A model of acceleration of Anomalous Cosmic Rays by Reconnection in the Heliosheath
• The density structure and star formation rate of non-isothermal polytropic turbulence
• A high-dispersion molecular gas component in nearby galaxies
• Stellar Populations in the Central 0.5 pc of the Galaxy I: A New Method for Constructing Luminosity Functions and Surface-Density Profiles
• Formation of Magnetized Prestellar Cores with Ambipolar Diffusion and Turbulence
• A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence
• Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation
• Gravitational Instabilities in Two-Component Galaxy Disks with Gas Dissipation
• The Impact of Modeling Assumptions in Galactic Chemical Evolution Models
• Molecular Cloud Populations in the Context of Their Host Galaxy Environments: A Multiwavelength Perspective
• Solar structure and evolution
• Central Regions of Barred Galaxies: Two-Dimensional Non-self-gravitating Hydrodynamic Simulations
• A Portrait of Cold Gas in Galaxies at 60pc Resolution and a Simple Method to Test Hypotheses That Link Small-Scale ISM Structure to Galaxy-Scale Processes
• Bar quenching in gas-rich galaxies
• Adiabatic Heating of Contracting Turbulent Fluids
• Planck Early Results: The submillimetre properties of a sample of Galactic cold clumps
• Balloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion
• Maximally Star-Forming Galactic Disks II. Vertically-Resolved Hydrodynamic Simulations of Starburst Regulation
• Quantifying Observational Projection Effects Using Molecular Cloud Simulations
• Nonthermal particles and photons in starburst regions and superbubbles
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• A new density variance - Mach number relation for subsonic and supersonic, isothermal turbulence
• Anchoring Magnetic Field in Turbulent Molecular Clouds
• Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
• Obtaining Spectra of Turbulent Velocity from Observations
• Star Formation in Disk Galaxies. II. The Effect of Star Formation and Photoelectric Heating on the Formation and Evolution of Giant Molecular Clouds
• The Sizes and Luminosities of Massive Star Clusters
• Graph-based interpretation of the Molecular Interstellar Medium Segmentation
• IN-SYNC II: Virial Stars from Sub-Virial Cores -- The Velocity Dispersion of Embedded Pre-Main-Sequence Stars in NGC 1333
• Statistical Description of Synchrotron Intensity Fluctuations: Studies of Astrophysical Magnetic Turbulence
• Lyman Radiation Hydrodynamics of Turbulent H II Regions in Molecular Clouds: A Physical Origin of LyC Leakage and the Associated Ly$\alpha$ Spectra
• Forming Super Star Clusters in the Central Starburst of NGC 253
• Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies
• Magnetic Field Amplification by Small-Scale Dynamo Action: Dependence on Turbulence Models and Reynolds and Prandtl Numbers
• Velocity Spectrum for HI at High Latitudes
• Is the PAMELA anomaly caused by the supernova explosions near the Earth?
• SPICY: The Spitzer/IRAC Candidate YSO Catalog for the Inner Galactic Midplane
• Protostellar birth with ambipolar and ohmic diffusion
• Polar alignment of a protoplanetary disk around an eccentric binary
• Dense core formation in supersonic turbulent converging flows
• Alignment Between Flattened Protostellar Infall Envelopes and Ambient Magnetic Fields
• The structures of embedded clusters in the Perseus, Serpens and Ophiuchus molecular clouds
• On the Kennicutt-Schmidt relation of low-metallicity high-redshift galaxies
• Physical Properties of Tidal Features in Interacting Disk Galaxies
• Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth
• HI as a Probe of the Large Scale Structure in the Post-Reionization Universe
• The Bolocam Galactic Plane Survey. XIV. Physical Properties of Massive Starless and Star Forming Clumps
• Algorithmic comparisons of decaying, isothermal, supersonic turbulence
• The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst
• An Excursion-Set Model for the Structure of GMCs and the ISM
• A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces: I. Cloud-scale Gas Motions
• Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Reprocessed Radiation Feedback from Nascent Super Star Clusters
• Strong biases in infrared-selected gravitational lenses
• The Musca cloud: A 6 pc-long velocity-coherent, sonic filament
• ALMA Resolves 30 Doradus: Sub-parsec Molecular Cloud Structure Near the Closest Super-Star Cluster
• CARMA Survey Toward Infrared-bright Nearby Galaxies (STING) II: Molecular Gas Star Formation Law and Depletion Time Across the Blue Sequence
• Evolution of supernovae-driven superbubbles with conduction and cooling
• Angular Momentum Transfer and Lack of Fragmentation in Self-Gravitating Accretion Flows
• Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
• Feeding SMBHs through supersonic turbulence and ballistic accretion
• Resolved Giant Molecular Clouds in Nearby Spiral Galaxies: Insights from the CANON CO (1-0) Survey
• Star Formation Laws and Efficiencies across 80 Nearby Galaxies
• Proper motions of the Arches cluster with Keck-LGS Adaptive Optics: the first kinematic mass measurement of the Arches
• ALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS0745-191
• Tsallis statistics as a tool for studying interstellar turbulence
• Molecular Cloud Evolution V. Cloud Destruction by Stellar Feedback
• Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• Monte Carlo Radiative Transfer
• PHIBSS: molecular gas, extinction, star formation and kinematics in the z=1.5 star forming galaxy EGS13011166
• Hall-effect Mediated Magnetic Flux Transport in Protoplanetary Disks
• The resolved stellar populations in the LEGUS galaxies
• Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation
• An Infrared through Radio Study of the Properties and Evolution of IRDC Clumps
• Turbulence-driven Polar Winds from T Tauri Stars Energized by Magnetospheric Accretion
• The Panchromatic Hubble Andromeda Treasury VIII: A Wide-Area, High-Resolution Map of Dust Extinction in M31
• Forming spectroscopic massive proto-binaries by disk fragmentation
• Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs
• Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago
• Molecular jets from low-mass young protostellar objects
• The Role of Magnetic Fields in Protostellar Outflows and Star Formation
• Evolution of Spin Direction of Accreting Magnetic Protostars and Spin-Orbit Misalignment in Exoplanetary Systems: II. Warped Discs
• A supersonic turbulence origin of Larson's laws
• Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way
• Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
• Impact of Protostellar Outflows on Turbulence and Star Formation Efficiency in Magnetized Dense Cores
• Gaia EDR3 Reveals the Substructure and Complicated Star Formation History of the Greater Taurus-Auriga Star Forming Complex
• Probing the evolution of molecular cloud structure II: From chaos to confinement
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• Feedback Effects on Low-Mass Star Formation
• New Tests for Disruption Mechanisms of Star Clusters: Methods and Application to the Antennae Galaxies
• Density Probability Distribution Functions in Supersonic Hydrodynamic and MHD Turbulence
• Disruption of giant molecular clouds and formation of bound star clusters under the influence of momentum stellar feedback
• Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
• The Mass-Size Relation from Clouds to Cores. I. A new Probe of Structure in Molecular Clouds
• Comparison of spectral slopes of magnetohydrodynamic and hydrodynamic turbulence and measurements of alignment effects
• ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results
• Moving mesh simulations of star forming cores in magneto-gravo-turbulence
• Investigations of Protostellar Outflow Launching and Gas Entrainment: Hydrodynamic Simulations and Molecular Emission
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure
• Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• Herschel/PACS Spectroscopic Survey of Protostars in Orion: The Origin of Far-Infrared CO Emission
• Inclination Evolution of Protoplanetary Disks Around Eccentric Binaries
• Field O stars: formed in situ or as runaways?
• A chemical solver to compute molecule and grain abundances and non-ideal MHD resistivities in prestellar core collapse calculations
• Dense cloud cores revealed by CO in the low metallicity dwarf galaxy WLM
• Efficiently Cooled Stellar Wind Bubbles in Turbulent Clouds II. Validation of Theory with Hydrodynamic Simulations
• The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds
• Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation
• An Exoplanet's Response to Anisotropic Stellar Mass-Loss During Birth and Death
• Millimeter-Wave Line Ratios and Sub-beam Volume Density Distributions
• Delving Deeper into the Tumultuous Lives of Galactic Dwarfs: Modeling Star Formation Histories
• Magnetization of cloud cores and envelopes and other observational consequences of reconnection diffusion
• Magnetized filamentary gas flows feeding the young embedded cluster in Serpens South
• Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman Observations
• The CARMA-NRO Orion Survey
• A High Resolution Study of the HI-H2 Transition across the Perseus Molecular Cloud
• Legacy of star formation in the pre-reionization universe
• A model for the formation of stellar associations and clusters from giant molecular clouds
• The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High Redshift
• Line Overlap and Self-Shielding of Molecular Hydrogen in Galaxies
• Spin alignment of stars in old open clusters
• The role of magnetic fields in the formation of protostellar discs
• Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes. I: Feedback-regulated Star Formation and Black Hole Growth
• Importance of the Initial Conditions for Star Formation - II. Fragmentation Induced Starvation and Accretion Shielding
• Testing Larson's relationships in massive clumps
• BLAST: The Mass Function, Lifetimes, and Properties of Intermediate Mass Cores from a 50 Square Degree Submillimeter Galactic Survey in Vela (l = ~265)
• Gas pile-up, gap overflow, and Type 1.5 migration in circumbinary disks: application to supermassive black hole binaries
• Spectrum and Anisotropy of Turbulence from Multi-Frequency Measurement of Synchrotron Polarization
• Preserving chemical signatures of primordial star formation in the first low-mass stars
• The importance of magnetic fields for the initial mass function of the first stars
• The origin of physical variations in the star formation law
• Searching for a link between the magnetic nature and other observed properties of Herbig Ae/Be stars and stars with debris disks
• First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf
• The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Perseus Protostars. VI. Characterizing the Formation Mechanism for Close Multiple Systems
• The Bolocam Galactic Plane Survey V: HCO+ and N2H+ Spectroscopy of 1.1 mm Dust Continuum Sources
• Stochastic self-enrichment, pre-enrichment, and the formation of globular clusters
• A Toomre-like stability criterion for the clumpy and turbulent interstellar medium
• A dynamical model of supernova feedback: gas outflows from the interstellar medium
• The structure of the thermally bistable and turbulent atomic gas in the local interstellar medium
• The SWELLS survey - V. A Salpeter stellar initial mass function in the bulges of massive spiral galaxies
• There is no magnetic braking catastrophe: Low-mass star cluster and protostellar disc formation with non-ideal magnetohydrodynamics
• Disruption of Molecular Clouds by Expansion of Dusty H II Regions
• Change of Magnetic Field$-$Gas Alignment at Gravity-Driven Alfvénic Transition in Molecular Clouds: Implications for Dust Polarization Observations
• GRB 120521C at z~6 and the Properties of High-redshift GRBs
• Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
• The Evolution of Massive YSOs in the LMC: Part I. Identification and Spectral Classification
• Evidence for a non-universal Kennicutt-Schmidt relationship using hierarchical Bayesian linear regression
• The First Galaxies: Assembly under Radiative Feedback from the First Stars
• Gas dynamics in the Milky Way: a low pattern speed model
• Shock Breakout in Type II Plateau Supernovae: Prospects for High Redshift Supernova Surveys
• Cloud and Star Formation in Disk Galaxy Models with Feedback
• Physical Processes in Star Formation
• Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design, Data Processing, and Spectral Analysis Methods
• Pressure Relations and Vertical Equilibrium in the Turbulent, Multiphase ISM
• CO line emission from galaxies in the Epoch of Reionization
• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region
• Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry
• Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24
• An Alternative Accurate Tracer of Molecular Clouds: The "$X_{\mathrm{CI}}$-Factor"
• The VLA Nascent Disk and Multiplicity Survey of Perseus Protostars (VANDAM). V. 18 Candidate Disks around Class 0 and I Protostars in the Perseus Molecular Cloud
• Alignment Between Protostellar Outflows and Filamentary Structure
• WARPFIELD 2.0: Feedback-regulated minimum star formation efficiencies of giant molecular clouds
• Giant molecular clouds and massive star formation in the southern milky way
• Radioactive 26Al from the Scorpius-Centaurus Association
• The Evolution and Properties of Rotating Massive Star Populations
• CARMA Survey Toward Infrared-bright Nearby Galaxies (STING): Molecular Gas Star Formation Law in NGC4254
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• The formation and dynamical evolution of young star clusters
• The Star Formation Rate of the Milky Way as seen by Herschel
• Outflow Driven Turbulence in Molecular Clouds
• The Nature of the Velocity Field in Molecular Clouds. I. The Non-Magnetic Case
• CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
• On the simultaneous evolution of massive protostars and their host cores
• The EDGE-CALIFA survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
• Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail
• The ALMA view of GMCs in NGC 300: Physical Properties and Scaling Relations at 10 pc Resolution
• The structure and statistics of interstellar turbulence
• Wind bubbles within H II regions around slowly moving stars
• Relative Alignment Between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud using Low and High Density Tracers
• The most metal-poor damped Lyman alpha systems: An insight into dwarf galaxies at high redshift
• The Effects of Magnetic Fields and Protostellar Feedback on Low-mass Cluster Formation
• Observational Diagnostics of Self-Gravitating MHD Turbulence in Giant Molecular Clouds
• The turbulent formation of stars
• On the stability of radiation-pressure-dominated cavities
• Magnetic Field Amplification in Young Galaxies
• Formation of the first stars and black holes
• The Formation and Evolution of Wide-Orbit Stellar Multiples In Magnetized Clouds
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• Molecular outflows towards O-type young stellar objects
• ALMA detection of the rotating molecular disk wind from the young star HD 163296
• From diffuse gas to dense molecular cloud cores
• Nonlinear Evolution of Global Hydrodynamic Shallow-Water Instability in Solar Tachocline
• Detection of a Bipolar Molecular Outflow Driven by a Candidate First Hydrostatic Core
• Distribution of velocity gradient orientations: Mapping magnetization with the Velocity Gradient Technique
• Investigating the inner discs of Herbig Ae/Be stars with CO bandhead and Br Gamma emission
• Primordial r-process Dispersion in Metal-Poor Globular Clusters
• High resolution studies of massive primordial haloes
• Properties of Interstellar Turbulence from Gradients of Linear Radio Polarization Maps
• An Evolutionary Model for Collapsing Molecular Clouds and Their Star Formation Activity
• On the formation of density filaments in the turbulent interstellar medium
• Damping of Alfven waves by Turbulence and its Consequences: from Cosmic-Rays Streaming to Launching Winds
• A Free-Form Prediction for the Reappearance of Supernova Refsdal in the Hubble Frontier Fields Cluster MACSJ1149.5+2223
• Anisotropic Formation of Magnetized Cores in Turbulent Clouds
• Implementation of Sink Particles in the Athena Code
• Supernova Feedback and the Hot Gas Filling Fraction of the Interstellar Medium
• Star Formation in the First Galaxies - II: Clustered Star Formation and the Influence of Metal Line Cooling
• Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements
• Matching dust emission structures and magnetic field in high-latitude cloud L1642: comparing Herschel and Planck maps
• The Herschel view of the on-going star formation in the Vela-C molecular cloud
• Ubiquitous velocity fluctuations throughout the molecular interstellar medium
• ALMA observations of fragmentation, sub-structure, and protostars in high-mass starless clump candidates
• On The Nature of Variations in the Measured Star Formation Efficiency of Molecular Clouds
• CO-dark molecular gas at high redshift: very large H${}_2$ content and high pressure in a low metallicity damped Lyman-alpha system
• CARMA Large Area Star Formation Survey: Structure and Kinematics of Dense Gas in Serpens Main
• A First Look at BISTRO Observations of The $\rho$ Oph-A core
• Structure of Stationary Strong Imbalanced Turbulence
• Review of Zeeman Effect Observations of Regions of Star Formation
• Magnetic Field Structure around Low-Mass Class 0 Protostars: B335, L1527 and IC348-SMM2
• How Universal is the SFR - H2 Relation?
• A physical model for the [CII]-FIR deficit in luminous galaxies
• MHD Turbulence
• Does the magnetic field suppress fragmentation in massive dense cores?
• Droplets I: Pressure-Dominated Sub-0.1 pc Coherent Structures in L1688 and B18
• The Fraction of Stars That Form in Clusters in Different Galaxies
• Unbound Young Stellar Systems: Star Formation on the loose
• The structure of the magnetic field in the massive star-forming region W75N
• Massive protostars as gamma-ray sources
• THOR - The HI, OH, Recombination Line Survey of the Milky Way - The pilot study: HI observations of the giant molecular cloud W43
• Magnetic Origins of the Stellar Mass-Obliquity Correlation in Planetary Systems
• Interstellar filaments and star formation
• Large scale IRAM 30m CO-observations in the giant molecular cloud complex W43
• The final data release of ALLSMOG: a survey of CO in typical local low-M* star-forming galaxies
• Do AGN outflows quench or enhance star formation?
• GMC Collisions as Triggers of Star Formation. II. 3D Turbulent, Magnetized Simulations
• The Formation of Stellar Clusters in Magnetized, Filamentary Infrared Dark Clouds
• Hierarchical fragmentation in the Perseus molecular cloud: From the cloud scale to protostellar objects
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: I. Turbulence Statistics
• Properties of dense cores in clustered massive star-forming regions at high angular resolution
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: II. Comparison with Observation, Clump Properties, and Scaling to Physical Units
• VLT/X-shooter spectroscopy of the GRB 120327A afterglow
• The chemical enrichment of the ICM from hydrodynamical simulations
• Can we explain AMS-02 antiproton and positron excesses simultaneously by nearby supernovae without pulsars nor dark matter?
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• Kinematics of OB-associations in Gaia epoch
• Zooming in on Individual Star Formation: Low- and High-mass Stars
• The HI-to-H2 Transition in a Turbulent Medium
• An ALMA Search for Substructure, Fragmentation, and Hidden Protostars in Starless Cores in Chamaeleon I
• Studying Turbulence from Doppler-broadened Absorption Lines: Statistics of Logarithms of Intensity
• The Razor's Edge of Collapse: The Transition Point from Lognormal to Powerlaw in Molecular Cloud PDFs
• The ALMA Survey of 70 $\mu \mathrm{m}$ Dark High-mass Clumps in Early Stages (ASHES). II: Molecular Outflows in the Extreme Early Stages of Protocluster Formation
• Molecular Outflows From the Protocluster, Serpens South
• The Bolocam Galactic Plane Survey. VIII. A Mid-Infrared Kinematic Distance Discrimination Method
• Star Clusters in Evolving Galaxies
• The EDGE-CALIFA survey: the influence of galactic rotation on the molecular depletion time across the Hubble sequence
• Strong magnetic fields detected in the cores of 11 red giant stars using gravity-mode period spacings
• Star formation in turbulent molecular clouds with colliding flow
• Evolution of linear warps in accretion discs and applications to protoplanetary discs in binaries
• Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks
• Gravitational instability in protostellar disks at low metallicities
• Helical Magnetic Fields in Molecular Clouds? A New Method to Determine the Line-of-Sight Magnetic Field Structure in Molecular Clouds
• The Importance of the Magnetic Field from an SMA-CSO-Combined Sample of Star-Forming Regions
• The Deuterium Fraction in Massive Starless Cores and Dynamical Implications
• The Turbulence Power Spectrum in Optically Thick Interstellar Clouds
• Protostar Formation in Supersonic Flows: Growth and Collapse of Spherical Cores
• On the formation of very metal-poor stars: The case of SDSS J1029151+172927
• Local Simulations of Spiral Galaxies with the TIGRESS Framework: I. Star Formation and Arm Spurs/Feathers
• Using CO line ratios to trace the physical properties of molecular clouds
• The Link Between the Formation Rates of Clusters and Stars in Galaxies
• Evidence for diffuse molecular gas and dust in the hearts of gamma-ray burst host galaxies
• Dense gas without star formation: The kpc-sized molecular disk in 3C326 N
• The resolved star-formation relation in nearby active galactic nuclei
• An Initial Mass Function for Individual Stars in Galactic Disks: I. Constraining the Shape of the IMF
• Chemical signatures of the first star clusters
• What sets the massive star formation rates and efficiencies of giant molecular clouds?
• Massive 70 micron quiet clumps II: non-thermal motions driven by gravity in massive star formation?
• From discs to planetesimals I: evolution of gas and dust discs
• Star cluster formation and cloud dispersal by radiative feedback: dependence on metallicity and compactness
• Hierarchical Structure of Magnetohydrodynamic Turbulence In Position-Position-Velocity Space
• Ultraviolet-Selected Field and Pre-Main-Sequence Stars Towards Taurus and Upper Scorpius
• How primordial magnetic fields shrink galaxies
• Physical constraints for the evolution of life on exoplanets
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• A $Herschel-SPIRE$ Survey of the Mon R2 Giant Molecular Cloud: Analysis of the Gas Column Density Probability Density Function
• Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields
• Angular Momentum in Giant Molecular Clouds. I. The Milky Way
• Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
• Gas Properties and Implications for Galactic Star Formation in Numerical Models of the Turbulent, Multiphase ISM
• The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A
• Measuring the Alfvenic Nature of the Interstellar Medium: Velocity Anisotropy Revisited
• Surviving infant mortality in the hierarchical merging scenario
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies
• The X-factor in Galaxies: II. The molecular hydrogen -- star formation relation
• Near Infrared Circular Polarization Images of NGC 6334-V
• Role of Cosmic Ray Streaming and Turbulent Damping in Driving Galactic Winds
• A Three-dimensional Simulation of a Magnetized Accretion Disk: Fast Funnel Accretion onto a Weakly Magnetized Star
• Scatter broadening of pulsars and implications on the interstellar medium turbulence
• Gas depletion in primordial globular clusters due to accretion onto stellar-mass black holes
• Young Stellar Objects and Triggered Star Formation in the Vulpecula OB Association
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• The Life and Death of Dense Molecular Clumps in the Large Magellanic Cloud
• Protostellar collapse: the conditions to form dust rich protoplanetary disks
• The Molecular Outflows in the rho Ophiuchi Main Cloud: Implications For Turbulence Generation
• Fragmentation, infall, and outflow around the showcase massive protostar NGC7538 IRS1 at 500 AU resolution
• Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
• Physical Properties of Dense Cores in the Rho Ophiuchi Main Cloud and A Significant Role of External Pressures in Clustered Star Formation
• Gradients of Synchrotron Polarization: Tracing 3D distribution of magnetic fields
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Polar alignment of a protoplanetary disc around an eccentric binary II: Effect of binary and disc parameters
• High Resolution 8 mm and 1 cm Polarization of IRAS 4A from the VLA Nascent Disk and Multiplicity (VANDAM) Survey
• Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
• The Degree of Fine-Tuning in our Universe -- and Others
• Effect of Angular Momentum Alignment and Strong Magnetic Fields on the Formation of Protostellar Disks
• The ATLASGAL survey: The sample of young massive cluster progenitors
• Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core
• Magnetic field morphology in nearby molecular clouds as revealed by starlight and submillimetre polarization
• CARMA Survey Toward Infrared-bright Nearby Galaxies (STING). III. The Dependence of Atomic and Molecular Gas Surface Densities on Galaxy Properties
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• Assembly of Protoplanetary Disks and Inclinations of Circumbinary Planets
• A catalogue of 74 new open clusters found in Gaia Data-Release 2
• Dust Polarization Toward Embedded Protostars in Ophiuchus with ALMA. II. IRAS 16293-2422
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• Modeling UV Radiation Feedback from Massive Stars: III. Escape of Radiation from Star-forming Giant Molecular Clouds
• Protostellar collapse simulations in spherical geometry with dust coagulation and fragmentation
• The Anatomy of the Column Density Probability Distribution Function (N-PDF)
• The CO-to-H2 Conversion Factor across the Perseus Molecular Cloud
• Very Large Array Observations of Ammonia in Infrared-Dark Clouds II: Internal Kinematics
• What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
• The fractal dimension of star-forming regions at different spatial scales in M33
• The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0
• Velocity Anisotropy as a Diagnostic of the Magnetization of the Interstellar Medium and Molecular clouds
• An Evolutionary Model for Collapsing Molecular Clouds and Their Star Formation Activity. II. Mass Dependence of the Star Formation Rate
• The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations
• Star formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regions
• Fragmentation in the First Galaxies
• Characterizing gravitational instability in turbulent multi-component galactic discs
• Outflows and Bubbles in Taurus: Star-formation Feedback Sufficient to Maintain Turbulence
• Magnetic Fields in the Formation of the First Stars. I. Theory vs. Simulation
• Indications of a sub-linear and non-universal Kennicutt-Schmidt relationship
• Physical properties and scaling relations of molecular clouds: the effect of stellar feedback
• The first galaxies: simulating their feedback-regulated assembly
• Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
• New insights on the Galactic Bulge Initial Mass Function
• Evolution of giant molecular clouds across cosmic time
• The Next Generation BLAST Experiment
• Resolving Gas Dynamics in the Circumnuclear Region of a Disk Galaxy in a Cosmological Simulation
• The Origin of OB Clusters: From 10 pc to 0.1 pc
• Characterizing the properties of cluster precursors in the MALT90 survey
• The Protostellar Mass Function
• Low energy cosmic rays
• The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP
• The Astrochemical Impact of Cosmic Rays in Protoclusters I: Molecular Cloud Chemistry
• Mapping the core mass function to the initial mass function
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• Widespread Molecular Outflows in the Infrared Dark Cloud G28.37+0.07: Indications of Orthogonal Outflow-Filament Alignment
• Probing the Protostellar Envelope around L1157: the Dust and Gas Connection
• An Early Transition to Magnetic Supercriticality in Star Formation
• Forced turbulence in thermally bistable gas: A parameter study
• New Open Cluster candidates Found in Galactic Disk Using Gaia DR2/EDR3 Data
• The Bolocam Galactic Plane Survey. XII. Distance Catalog Expansion Using Kinematic Isolation of Dense Molecular Cloud Structures With 13CO(1-0)
• Are Super-Luminous supernovae and Long GRBs produced exclusively in young dense star clusters?
• Polar alignment of a protoplanetary disc around an eccentric binary III: Effect of disc mass
• Chronology of star formation and disk evolution in the Eagle Nebula
• Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence
• Orbital dynamics of circumbinary planets
• Galactic interstellar turbulence in the southern sky seen through spatial gradients of the polarization vector
• Magnetic Fields and Infall Motions in NGC 1333 IRAS 4
• Reflections on nebulae around young stars: A systematic search for late-stage infall of material onto Class II disks
• The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations
• Confronting Outflow-Regulated Cluster Formation Model with Observations
• Impact of Winds from Intermediate-Mass Stars on Molecular Cloud Structure and Turbulence
• Low-Metallicity Protostars and the Maximum Stellar Mass Resulting from Radiative Feedback
• Lowering the Characteristic Mass of Cluster Stars by Magnetic Fields and Outflow Feedback
• Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
• CARMA Large Area Star Formation Survey: Project Overview with Analysis of Dense Gas Structure and Kinematics in Barnard 1
• Fossil magnetic field of accretion disks of young stars
• Alfvenic Turbulence Beyond the Ambipolar Diffusion Scale
• Prestellar Core Formation, Evolution, and Accretion from Gravitational Fragmentation in Turbulent Converging Flows
• The initial mass function of star clusters that form in turbulent molecular clouds
• The effect of episodic accretion on the phase transition of CO and CO_2 in low-mass star formation
• Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC18310-4
• Interstellar Sonic and Alfvénic Mach Numbers and the Tsallis Distribution
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Herschel-HIFI observations of high-J CO and isotopologues in star-forming regions: from low- to high-mass
• Resolving the Vela C ridge with P-ArTeMiS and Herschel
• Magnetized interstellar molecular clouds: II. The Large-Scale Structure and Dynamics of Filamentary Molecular Clouds
• Shock Waves and Energy Dissipation in Magnetohydrodynamic Turbulence
• ALMA-IMF VI -- Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• The Darkest Shadows: Deep Mid-Infrared Extinction Mapping of a Massive Protocluster
• Diversity of chemistry and excitation conditions in the high-mass star forming complex W33
• Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
• Magnetic fields in the massive dense cores of DR21 filament: weakly magnetized cores in a strongly magnetized filament
• Runaway OB Stars in the Small Magellanic Cloud: Dynamical Versus Supernova Ejections
• Formation of the Hub-Filament System G33.92+0.11: Local Interplay between Gravity, Velocity, and Magnetic Field
• Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties
• Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
• Gaseous Spiral Structure and Mass Drift in Spiral Galaxies
• WISE J080822.18-644357.3 - a 45 Myr-old accreting M dwarf hosting a primordial disc
• A Mid-Infrared Census of Star Formation Activity in Bolocam Galactic Plane Survey Sources
• Impact of X-rays on CO emission from high-z galaxies
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• Star Formation Stochasticity Measured from the Distribution of Burst Indicators
• Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium
• Star Formation in Nuclear Rings of Barred Galaxies
• Protostar Mass Due to Infall and Dispersal
• Dependence of $X_{\mathrm{CO}}$ on metallicity, intensity, and spatial scale in a self-regulated interstellar medium
• The simulation of molecular clouds formation in the Milky Way
• Effects of Disk Warping on the Inclination Evolution of Star-Disk-Binary Systems
• The CO-dark molecular gas mass in 30 Doradus
• The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
• On the Observed Diversity of Star Formation Efficiencies in Giant Molecular Clouds
• A quantification of the non-spherical geometry and accretion of collapsing cores
• Molecular Outflows Identified in the FCRAO CO Survey of the Taurus Molecular Cloud
• Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06" resolution
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• A switch to reduce resistivity in smoothed particle magnetohydrodynamics
• 3D magnetic field morphology of the Perseus molecular cloud
• Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
• Density Profiles in Molecular Cloud Cores Associated with High-Mass Star-Forming Regions
• 13CO Cores in Taurus Molecular Cloud
• GMC Collisions as Triggers of Star Formation. I. Parameter Space Exploration with 2D Simulations
• Distances and statistics of local molecular clouds in the first Galactic quadrant
• The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores
• A grid of 1D low-mass star formation collapse models
• Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas
• Molecular Tracers of Turbulent Shocks in Giant Molecular Clouds
• Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
• Understanding the origin of the magnetic field morphology in the wide-binary protostellar system BHR 71
• Isothermal Fragmentation: Is there a low-mass cut-off?
• Near-Infrared Imaging Polarimetry of the Serpens Cloud Core: Magnetic Field Structure, Outflows, and Inflows in A Cluster Forming Clump
• Galactic H2CO Densitometry I: Pilot survey of Ultracompact HII regions and methodology
• The Multi-phase Turbulence Density Power Spectra in the Perseus Molecular Cloud
• An indirect measurement of gas evolution in galaxies at $0.5\le z\le 2.0$
• The stellar population and initial mass function of NGC 1399 with MUSE
• Energy budget of forming clumps in numerical simulations of collapsing clouds
• A statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores
• Testing kinematic distances under a realistic Galactic potential
• Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC+ and comparing with simulation
• On the distribution of protostar masses
• Giant molecular clouds in the non-grand design spiral galaxy NGC 6946
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Slow Star Formation in the Milky Way: Theory Meets Observations
• Synthetic observations of star formation and the interstellar medium
• First Core Properties: From Low- to High-mass Star Formation
• Study of velocity centroids based on the theory of fluctuations in position-position-velocity space
• Turbulence, Coherence and Collapse: Three Phases for Core Evolution
• Synthetic Observations of Magnetic Fields in Protostellar Cores
• The Clustering Behavior of Pre-Main Sequence Stars in NGC 346 in the Small Magellanic Cloud
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• Star Formation in Molecular Clouds
• The volumetric star formation law for nearby galaxies -- Extension to dwarf galaxies and low-density regions
• Physical Properties of the star-forming clusters in NGC 6334
• The volumetric star formation law in the Milky Way
• Dual Effects of Ram Pressure on Star Formation in Multi-phase Disk Galaxies with Strong Stellar Feedback
• Isotropically Driven versus Outflow Driven Turbulence: Observational Consequences for Molecular Clouds
• Jeans instability criterion modified by external tidal field
• The effect of ISM turbulence on the gravitational instability of galactic discs
• The HI Probability Distribution Function and the Atomic-to-Molecular Transition in Molecular Clouds
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• Simulations of cosmic ray propagation
• Acceleration of polytropic solar wind: Parker Solar Probe observation and one-dimensional model
• Magnetic field strength from turbulence theory (I): Using differential measure approach (DMA)
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• Directly observing continuum emission from self-gravitating spiral waves
• Radiation Transfer of Models of Massive Star Formation. II. Effects of the Outflow
• Protostellar collapse and fragmentation using an MHD GADGET
• Accretion bursts in young stars driven by cluster environment
• Revealing Gravitational Collapse in Serpens G3-G6 Molecular Cloud using Velocity Gradients
• The Galactic Census of High- and Medium-mass Protostars. II. Luminosities and Evolutionary States of a Complete Sample of Dense Gas Clumps
• Circumbinary disk inner radius as a diagnostic for disk--binary misalignment
• The Panchromatic Hubble Andromeda Treasury IV. A Probabilistic Approach to Inferring the High Mass Stellar Initial Mass Function and Other Power-law Functions
• Effects of metal enrichment and metal cooling in galaxy growth and cosmic star formation history
• A SiO J = 5 - 4 Survey Toward Massive Star Formation Regions
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• A model for the onset of self-gravitation and star formation in molecular gas governed by galactic forces: II. the bottleneck to collapse set by cloud-environment decoupling
• The Lesser Role of Shear in Star Formation: Insight from the Galactic Ring Survey
• Lyα emission from galaxies in the Epoch of Reionization
• ALMA-IRDC: Dense gas mass distribution from cloud to core scales
• The history of the dark and luminous side of Milky Way-like progenitors
• Modeling the Atomic-to-Molecular Transition and Chemical Distributions of Turbulent Star-Forming Clouds
• Evolution of Blister-Type HII Regions in a Magnetized Medium
• Magnetic field fluctuations in anisotropic, supersonic turbulence
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• The Formation of Very Massive Stars
• The molecular gas content of the Pipe Nebula I. Direct evidence of outflow-generated turbulence in B59?
• The role of stellar collisions for the formation of massive stars
• Multiple Star Systems in the Orion Nebula
• Mixing of metals during star cluster formation: statistics and implications for chemical tagging
• Technique for separating velocity and density contributions in spectroscopic data and its application to studying turbulence and magnetic fields
• Formation of the First Low-Mass Stars from Cosmological Initial Conditions
• Temperature structure and kinematics of the IRDC G035.39-00.33
• Energy transfer in compressible magnetohydrodynamic turbulence for isothermal self-gravitating fluids
• TurbuStat: Turbulence Statistics in Python
• Star formation in the first galaxies - III. Formation, evolution, and characteristics of the first stellar cluster
• Giant protostellar flares: accretion-driven accumulation and reconnection-driven ejection of magnetic flux in protostars
• Simulations of momentum feedback by black hole winds
• Bondi-Hoyle Accretion in an Isothermal Magnetized Plasma
• Methanol masers probing the ordered magnetic field of W75N
• Non-ideal magnetohydrodynamics vs turbulence I: Which is the dominant process in protostellar disc formation?
• Stellar dynamics in gas: The role of gas damping
• Geometry, Kinematics, and Magnetization of Simulated Prestellar Cores
• The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I
• Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
• Multi-scale dynamics in star-forming regions: the interplay between gravity and turbulence
• Cloud formation in the atomic and molecular phase: HI self absorption (HISA) towards a Giant Molecular Filament
• Alignment and rotational disruption of dust
• Characterization of Molecular Outflows in The Substellar Domain
• Magnetic fields in the formation of the first stars.--II Results
• Herbig Stars: A Quarter Century of Progress
• On the stability of non-isothermal Bonnor-Ebert spheres
• Velocity Gradient in the Presence of Self-Gravity: Identifying Gravity-induced Inflow and Determining Collapsing Stage
• Probing Episodic Accretion in Very Low Luminosity Objects
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane
• Dynamical Gaseous Rings in Global Simulations of Protoplanetary Disk Formation
• Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies
• The Giant Molecular Cloud Environments of Infrared Dark Clouds
• Structure and Fragmentation of a high line-mass filament: Nessie
• The DiskMass Survey. VIII. On the Relationship Between Disk Stability and Star Formation
• High-mass star formation at sub-50AU scales
• Two Thresholds for Globular Cluster Formation and their Dominance of Star Formation in the Early-Universe
• Physics of Coevolution of Galaxies and Supermassive Black Holes
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Large-scale magnetic fields in Bok globules
• The Origin of Interstellar Turbulence in M33
• Physics in Very Strong Magnetic Fields: Introduction and Overview
• Asymmetric Line Profiles in Dense Molecular Clumps Observed in MALT90: Evidence for Global Collapse
• First Time-dependent Study of H2 and H3+ Ortho-Para Chemistry in the Diffuse Interstellar Medium: Observations Meet Theoretical Predictions
• The JCMT BISTRO survey: alignment between outflows and magnetic fields in dense cores/clumps
• Turbulent Magnetic Field Amplification by the Interaction of Shock Wave and Inhomogeneous Medium
• Terrestrial planet formation: Dynamical shake-up and the low mass of Mars
• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• A simple model for molecular hydrogen chemistry coupled to radiation hydrodynamics
• Star formation in dense clusters
• Mach number study of supersonic turbulence: The properties of the density field
• Shock generated vorticity in the interstellar medium and the origin of the stellar initial mass function
• Origin and Evolution of Saturn's Ring System
• Measuring Turbulence with Young Stars in the Orion Complex
• Nobeyama 45-m mapping observations toward nearby molecular clouds, Orion A, Aquila Rift, and M17: Project overview
• The relation between atomic gas and star formation rate densities in faint irregular galaxies
• Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
• Scaling relations of the properties for CO resolved structures in nearby spiral galaxies
• A large-scale CO survey of the Rosette Molecular Cloud: assessing the effects of O stars on surrounding molecular gas
• Empirical modelling of the BLASTPol achromatic half-wave plate for precision submillimetre polarimetry
• CO excitation in the Seyfert galaxy NGC 34: stars, shock or AGN driven?
• Fast Magnetic Reconnection and Energetic Particle Acceleration
• Deuterium Fractionation as an Evolutionary Probe in Massive Proto-stellar/cluster Cores
• Anisotropies in Compressible MHD Turbulence: Probing Magnetic Fields and Measuring Magnetization
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• The IMF as a function of supersonic turbulence
• Angular momentum transfer in primordial discs and the rotation of the first stars
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. I. The unmagnetized and zero-feedback limit
• Turbulence in a self-gravitating molecular cloud core
• Tracing the ISM magnetic field morphology: The potential of multi-wavelength polarization measurements
• Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloud
• Formation and evolution of planetary systems: the impact of high angular resolution optical techniques
• Oort cloud Ecology II: The chronology of the formation of the Oort cloud
• The Forgotten Quadrant Survey. ${}^{12}$CO and ${}^{13}$CO (1-0) survey of the Galactic Plane in the range 220°$<l<$240° -2.5°$<b<$0°
• Non-linear Evolution of Rayleigh-Taylor Instability in a Radiation Supported Atmosphere
• Chemical Abundances in a Turbulent Medium -- H${}_2$, OH${}^{+}$, H${}_2$O${}^{+}$, ArH${}^{+}$
• Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
• Formation of the first stars
• Discovery of the Zeeman Effect in the 44 GHz Class I methanol maser line
• A New Method to Trace Three-dimensional Magnetic Field Structure within Molecular Clouds Using Dust Polarization
• Shock-multicloud interactions in galactic outflows -- I. Cloud layers with log-normal density distributions
• Multicolor Variability of Young Stars in the Lagoon Nebula: Driving Causes and Intrinsic Timescales
• Damping of MHD turbulence in partially ionized gas and the observed difference of velocities of neutrals and ions
• Birth of convective low-mass to high-mass second Larson cores
• Giant Molecular Cloud Formation in Disk Galaxies: Characterizing Simulated versus Observed Cloud Catalogues
• On the turbulence driving mode of expanding HII regions
• Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
• Flux Correlations in Supersonic Isothermal Turbulence
• The Initial Core Mass Function due to Ambipolar Diffusion in Molecular Clouds
• A New Way to Conserve Total Energy for Eulerian Hydrodynamic Simulations with Self-Gravity
• The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence
• A general hybrid radiation transport scheme for star formation simulations on an adaptive grid
• Hydrodynamical simulations and semi-analytic models of galaxy formation: two sides of the same coin
• Formation of globular clusters in dwarf galaxies of the Local Group
• Linewidth Differences of Neutrals and Ions Induced by MHD Turbulence
• The Formation and Evolution of Small Star Clusters
• W49A: A starburst triggered by expanding shells
• MHD Turbulence, Turbulent Dynamo and Applications
• Multi-epoch Sub-arcsecond [Fe II] Spectroimaging of the DG Tau Outflows with NIFS. I. First data epoch
• Optical/Near-IR Polarization Survey of Sh 2-29: Magnetic Fields, Dense Cloud Fragmentations and Anomalous Dust Grain Sizes
• Quantifying the Universality of the Stellar Initial Mass Function in Old Star Clusters
• Review of scientific topics for Millimetron space observatory
• Piecewise Parabolic Method on a Local Stencil for Magnetized Supersonic Turbulence Simulation
• The Rotating Molecular Structures and the Ionized Outflow Associated with IRAS 16547-4247
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• Radio Synchrotron Fluctuation Statistics as a Probe of Magnetized Interstellar Turbulence
• Self-gravity in neutrino-dominated accretion disks
• The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star Forming Galaxies from z~1 to z~3
• Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds
• High-resolution APEX/LAsMA ${}^{12}$CO and ${}^{13}$CO (3-2) observation of the G333 giant molecular cloud complex : I. Evidence for gravitational acceleration in hub-filament systems
• Nobeyama 45-m Mapping Observations toward Orion A.I. Molecular Outflows
• The photometric variability of massive stars due to gravity waves excited by core convection
• Constraining a Model of Turbulent Coronal Heating for AU Microscopii with X-Ray, Radio, and Millimeter Observations
• Distributions of Short-Lived Radioactive Nuclei Produced by Young Embedded Stellar Clusters
• Low Frequency Carbon Radio Recombination Lines I: Calculations of Departure Coefficients
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Polarimetric studies of magnetic turbulence with interferometer
• Dust clearing by radial drift in evolving protoplanetary discs
• Supernovae feedback propagation: the role of turbulence
• Effects of initial density profiles on massive star cluster formation in giant molecular clouds
• Star-disk alignment in the protoplanetary disks: SPH simulation of the collapse of turbulent molecular cloud cores
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies III. Structure and Dynamics of Filaments and Clumps in Giant Molecular Clouds
• Dynamical cloud formation traced by atomic and molecular gas
• Star Formation & Young Stellar Content in the W3 GMC
• Probing the physics of star formation (ProPStar): I. First resolved maps of the electron fraction and cosmic-ray ionization rate in NGC 1333
• Two-phase model for Black Hole feeding and feedback
• Star Formation in Disk Galaxies. III. Does stellar feedback result in cloud death?
• Compressible turbulence in the interstellar medium: New insights from a high-resolution supersonic turbulence simulation
• Curvature of magnetic field lines in compressible magnetized turbulence: Statistics, magnetization predictions, gradient curvature, modes and self-gravitating media
• Assessing the Performance of Molecular Gas Clump Identification Algorithms
• HST-Scale 3D simulations of MHD disc winds : A rotating two-component jet structure
• The clustered nature of star formation. Pre--main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud
• Global dynamics of the interstellar medium in magnetised disc galaxies
• Alignment of Protostars and Circumstellar Disks During the Embedded Phase
• Effects of dust absorption on spectroscopic studies of turbulence
• Modeling the accretion disk around the high-mass protostar GGD 27-MM1
• Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust
• Young and intermediate-age massive star clusters
• The Gas Properties of the W3 GMC: A HARP study
• Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium
• AGN impact on the molecular gas in galactic centers as probed by CO lines
• On the gravitational content of molecular clouds and their cores
• Studying Magnetohydrodynamic Turbulence with Synchrotron Polarization Dispersion
• An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
• Massive Star Formation of the Sgr A East HII Regions Near the Galactic Center
• The Simons Observatory: Galactic Science Goals and Forecasts
• The Elephant in the Room: The Importance of Where and When Massive Stars Form in Molecular Clouds
• Cloud formation in colliding flows: influence of the choice of cooling function
• Galactic foregrounds: Spatial fluctuations and a procedure of removal
• Statistical tracing of magnetic fields: comparing and improving the techniques
• Collapse of Turbulent Cores and Reconnection Diffusion
• The Galactic Census of High- and Medium-mass Protostars. IV. Molecular Clump Radiative Transfer, Mass Distributions, Kinematics, and Dynamical Evolution
• Disc population synthesis: Decrease in the solid mass reservoir through pebble drift
• First phase space portrait of a hierarchical stellar structure in the Milky Way
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• Molecular gas cloud properties at $z\simeq 1$ revealed by the superb angular resolution achieved with ALMA and gravitational lensing
• Wobbling and precessing jets from warped disks in binary systems
• Anomalous CO2 Ice Toward HOPS-68: A Tracer of Protostellar Feedback
• The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D
• The driving of turbulence in simulations of molecular cloud formation and evolution
• Formation of proto-cluster: a virialized structure from gravo-turbulent collapse II. A two-dimensional analytical model for rotating and accreting system
• A semi-analytic model of the turbulent multi-phase interstellar medium
• Radiative Supernova Remnants and Supernova Feedback
• CO excitation in the Seyfert galaxy NGC7130
• The CARMA-NRO Orion Survey: Protostellar Outflows, Energetics, and Filamentary Alignment
• Exploring star formation using the filaments in the Sloan Digital Sky Survey Data Release Five (SDSS DR5)
• PHIBSS: Exploring the Dependence of the CO-H${}_2$ Conversion Factor on Total Mass Surface Density at $z<1.5$
• Molecular cloud distances based on the MWISP CO survey and Gaia DR2
• A scaling relation for the molecular cloud lifetime in Milky Way-like galaxies
• Statistical properties of galactic CMB foregrounds: dust and synchrotron
• Molecular cloud formation by compression of magnetized turbulent gas subjected to radiative cooling
• Can the observed E/B ratio for dust galactic foreground be explained by sub-Alfvenic turbulence?
• EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions III. The flux-limited sample
• The Dense Filamentary Giant Molecular Cloud G23.0-0.4: Birthplace of Ongoing Massive Star Formation
• Ambipolar Diffusion Heating in Turbulent Systems
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• Gravity Versus Magnetic Fields in Forming Molecular Clouds
• CMZoom II: Catalog of Compact Submillimeter Dust Continuum Sources in the Milky Way's Central Molecular Zone
• Wave Decay in MHD Turbulence
• FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). VI. Dense gas and mini-starbursts in the W43 giant molecular cloud complex
• Beyond the pseudo-time-dependent approach: chemical models of dense core precursors
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• Local stability of a gravitating filament: a dispersion relation
• The VMC Survey XXII. Hierarchical Star Formation in the 30 Doradus-N158-N159-N160 Star-Forming Complex
• Galactic Spiral Shocks with Thermal Instability in Vertically Stratified Galactic Disks
• Magnetic Field Structure in Spheroidal Star-Forming Clouds
• Simulating Supersonic Turbulence in Magnetized Molecular Clouds
• SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
• Star formation efficiencies of molecular clouds in a galactic center environment
• Ambipolar Diffusion in Action: Transient C shock Structure and Prestellar Core Formation
• From large scale gas compression to cluster formation in the Antennae overlap region
• A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence
• A 2-3 mm high-resolution molecular line survey towards the centre of the nearby spiral galaxy NGC 6946
• The Milky Way Project and ATLASGAL: The distribution and physical properties of cold clumps near infrared bubbles
• Distortion of Magnetic Fields in a Starless Core: Near-Infrared Polarimetry of FeSt 1-457
• CO Multi-line Imaging of Nearby Galaxies (COMING): VI. Radial variations in star formation efficiency
• The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
• A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gas
• Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium
• The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds
• The CH+ Abundance in Turbulent, Diffuse Molecular Clouds
• SHELS: Optical Spectral Properties of WISE 22 μm-selected Galaxies
• The Velocity Statistics of Turbulent Clouds in the Presence of Gravity, Magnetic fields, Radiation, and Outflow Feedback
• Stellar Spins in the Open Cluster NGC 2516
• Molecular Cloud Cores with High Deuterium Fraction: Nobeyama Single-Pointing Survey
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• A molecular absorption line survey toward the AGN of Hydra-A
• The role of initial magnetic field structure in the launching of protostellar jets
• Producing Synthetic Maps of Dust Polarization using Velocity Channel Gradient Technique
• Dense molecular cocoons in the massive protocluster W3 IRS5: a test case for models of massive star formation
• "Starless" Super-Jeans Cores in Four Gould Belt Clouds
• From Gas to Stars in Energetic Environments: Dense Gas Clumps in the 30 Doradus Region Within the Large Magellanic Cloud
• A Map of Diffuse Radio Emission at 182 MHz to Enhance Epoch of Reionization Observations in the Southern Hemisphere
• On the Origin of the Salpeter Slope for the Initial Mass Function
• The Metallicity Dependence of the HI Shielding Layers in Nearby Galaxies
• OH absorption in the first quadrant of the Milky Way as seen by THOR
• An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
• Role of magnetic fields in fueling Seyfert nuclei
• Nonlinear turbulent dynamo during gravitational collapse
• VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies
• Dimensional argument for the impact of turbulent support on the stellar initial mass function
• Disruption of Star Clusters in the Interacting Antennae Galaxies
• Star-forming filament models
• The Davis-Chandrasekhar-Fermi Method Revisited
• LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
• Substellar-Mass Condensations in Prestellar Cores
• The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
• PHANGS: Constraining Star Formation Timescales Using the Spatial Correlations of Star Clusters and Giant Molecular Clouds
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• Estimating the molecular gas mass of low-redshift galaxies from a combination of mid-infrared luminosity and optical properties
• Properties and selected implications of magnetic turbulence for interstellar medium, Local Bubble and solar wind
• Earliest Stages of Protocluster Formation: Substructure and Kinematics of Starless Cores in Orion
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• Nonuniversal interstellar density spectra probed by pulsars
• Measuring magnetization with rotation measures and velocity centroids in supersonic MHD turbulence
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Synthetic observations of first hydrostatic cores in collapsing low-mass dense cores II. Simulated ALMA dust emission maps
• Characterizing the Turbulent Properties of the Starless Molecular Cloud MBM16
• Cosmological simulations of Milky Way-sized galaxies
• The alignment of the polarization of HAe/Be stars with the interstellar magnetic field
• A hybrid SPH/N-body method for star cluster simulations
• Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
• The Supershell-Molecular Cloud Connection: Large-Scale Stellar Feedback and the Formation of the Molecular ISM
• Formation of Terrestrial Planets
• Identifying Tools for Comparing Simulations and Observations of Spectral-line Data Cubes
• The Effect of Turbulence on Nebular Emission Line Ratios
• Reconciling the GRB rate and star formation histories
• ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
• A possible observational bias in the estimation of the virial parameter in virialized clumps
• Star Formation in a Turbulent Framework: From Giant Molecular Clouds to Protostars
• Multi-scale physical properties of NGC 6334 as revealed by local relative orientations between magnetic fields, density gradients, velocity gradients, and gravity
• Mapping of the structure of the galactic magnetic field with velocity gradients: Test using star light polarization
• Sustaining star formation rates in spiral galaxies - Supernova-driven turbulent accretion disk models applied to THINGS galaxies
• Globular Clusters in High-Redshift Dwarf Galaxies: A Case Study from the Local Group
• Spectral properties of magnetohydrodnamic turbulence revealed by polarization synchrotron emission with Faraday rotation
• Is SS 433 a misaligned ultraluminous X-ray source? Constraints from its reflected signal in the Galactic plane
• The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
• Embedded Young Massive Star Clusters in the Antennae Merger
• Evidence for Dynamically Important Magnetic Fields in Molecular Clouds
• Non-adiabatic turbulence driving during gravitational collapse
• Simultaneous evidence of edge collapse and hub-filament configurations: A rare case study of a Giant Molecular Filament G45.3+0.1
• Testing 24 micron and Infrared Luminosity as Star Formation Tracers for Galactic Star Forming Regions
• Physical Modeling of Dust Polarization from Magnetically Enhanced Radiative Torque (MRAT) Alignment in Protostellar Cores with POLARIS
• Alignment of the magnetic field in star forming regions and why it might be difficult to observe
• Magnetic Field Orientation in Self-Gravitating Turbulent Molecular Clouds
• Exact relations for energy transfer in self-gravitating isothermal turbulence
• Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?
• Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
• The birth and early evolution of a low mass protostar
• When is star formation episodic? A delay differential equation negative feedback model
• Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation
• Extremely Dense Cores associated with Chandra Sources in Ophiuchus A: Forming Brown Dwarfs Unveiled?
• Expanding CO Shells in the Orion A Molecular Cloud
• The Early Stage of Molecular Cloud Formation by Compression of Two-phase Atomic Gases
• Incidence of HI 21-cm absorption in strong FeII systems at $0.5<z<1.5$
• An All-Sky Sample of Intermediate-Mass Star-Forming Regions
• Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
• The Interstellar Medium and Star Formation of Galactic Disks. I. ISM and GMC properties with Diffuse FUV and Cosmic Ray Backgrounds
• Large-eddy simulations of isolated disc galaxies with thermal and turbulent feedback
• Investigating the Complex Velocity Structures within Dense Molecular Cloud Cores with GBT-Argus
• The driving scale -- density decorrelation scale relation in a turbulent medium
• Physical and chemical structure of the Serpens filament -- fast formation and gravity-driven accretion
• A Spitzer Space Telescope survey of massive young stellar objects in the G333.2-0.4 giant molecular cloud
• Physical and chemical modeling of the starless core L1512
• The Effects of Inhomogeneities within Colliding Flows on the Formation and Evolution of Molecular Clouds
• A New Method for Constraining Molecular Cloud Thickness: A study of Taurus, Perseus and Ophiuchus
• Astrochemical Correlations in Molecular Clouds
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• On the Origin of the High Column Density Turnover in the HI Column Density Distribution
• Equilibrium Star Formation In A Constant Q Disk: Model Optimisation and Initial Tests
• Radiatively Efficient Magnetized Bondi Accretion
• A young stellar cluster within the RCW41 HII region: deep NIR photometry and Optical/NIR polarimetry
• Testing the Turbulent Origin of the Stellar Initial Mass Function
• A Comparative Astrochemical Study Of The High-Mass Protostellar Objects NGC 7538 IRS 9 and IRS 1
• Formation of the SDC13 Hub-Filament System: A Cloud-Cloud Collision Imprinted on The Multiscale Magnetic Field
• Can the Growth of Dust Grains in Low-Metallicity Star-Forming Clouds Affect the Formation of Metal-Poor Low-Mass Stars?
• Probing the intergalactic turbulence with fast radio bursts
• The eclipse of the V773 Tau B circumbinary disk
• Studies of Turbulence Dissipation in Taurus Molecular Cloud with Core Velocity Dispersion (CVD)
• Synthetic Observations of the Evolution of Starless Cores in a Molecular Cloud Simulation: Comparisons with JCMT Data and Predictions for ALMA
• Effect of feedback of massive stars in the fragmentation, distribution, and kinematics of the gas in two star forming regions in the Carina Nebula
• Non-Equilibrium Chemistry of Dynamically Evolving Prestellar Cores: II. Ionization and Magnetic Field
• HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
• G30.79~FIR~10: A gravitationally bound infalling high-Mass star forming clump
• Reproducing the CO-to-H${}_2$ conversion factor in cosmological simulations of Milky Way-mass galaxies
• Dense Cores, Filaments and Outflows in the S255IR Region of High Mass Star Formation
• Signatures of fast and slow magnetohydrodynamic shocks in turbulent molecular clouds
• The link between solenoidal turbulence and slow star formation in G0.253+0.016
• Collapse and fragmentation of molecular clouds under pressure
• Chemical evolution of giant molecular clouds in simulations of galaxies
• A Highly collimated Water Maser Bipolar Outflow in the Cepheus A HW3d Massive Young Stellar Object
• A Survey for Hydroxyl in the THOR Pilot Region around W43
• Implementation of stellar heating feedback in simulations of star cluster formation: effects on the initial mass function
• Gas Column Density Distribution of Molecular Clouds in the Third Quadrant of the Milky Way
• Global Collapses and Expansions in Star-Forming Clouds
• Study Turbulence and Probe Magnetic Field Using Gradients Technique: Application to HI-to-H2 Transition Regions
• Can Sgr A* flares reveal the molecular gas density PDF?
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. IV. Regulation of Galactic Star Formation Rates by Stellar Feedback
• Achieving Fast Reconnection in Resistive MHD Models via Turbulent Means
• Solid H2 in the interstellar medium
• HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules -- I. Survey description and a first look toward W3(OH), W3 IRS5 and NGC 7538 IRS1
• CARMA Large Area Star Formation Survey: Dense Gas in the Young L1451 Region of Perseus
• On the origin of the peak of the stellar initial mass function: exploring the tidal screening theory
• The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
• EVN observations of 6.7-GHz methanol maser polarization in massive star-forming regions II. First statistical results
• Baryon-dark matter scattering and first star formation
• Velocity Gradients: Magnetic Field Tomography towards the Supernova Remnant W44
• Physical effects on compact high-velocity clouds in the circumgalactic medium
• Droplets II: Internal Velocity Structures and Potential Rotational Motions in Pressure-dominated Coherent Structures
• How vortices and shocks provide for a flux loop in two-dimensional compressible turbulence
• Formation and spatial distribution of hypervelocity stars in AGN outflows
• On the shape of the mass-function of dense clumps in the Hi-GAL fields. I. SED determination and global properties of the mass-functions
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• GMC Collisions as Triggers of Star Formation. VI. Collision-Induced Turbulence
• Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse
• Spectral Energy Distributions of High Mass Proto Stellar Objects - Evidence for High Accretion Rates
• Low Frequency Carbon Radio Recombination Lines II: The Diffuse Interstellar Medium
• Effects of turbulence and rotation on protostar formation as a precursor to seed black holes
• Ultra Violet Escape Fractions from Giant Molecular Clouds During Early Cluster Formation
• Dense Regions in Supersonic Isothermal Turbulence
• Effects of Spiral Arms on Star Formation in Nuclear Rings of Barred-spiral Galaxies
• Molecular cloud catalogue from ${}^{13}$CO(1-0) data of the Forgotten Quadrant Survey
• PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction, $R_{\mathrm{mol}}$
• Pillars of creation amongst destruction: Star formation in molecular clouds near R136 in 30 Doradus
• A new method for measuring the 3D turbulent velocity dispersion of molecular clouds
• The small and the beautiful: How the star formation law affects galactic disk structure
• Effects of Grain Alignment Efficiency on Synthetic Dust Polarization Observations of Molecular Clouds
• Anchoring Magnetic Fields in Turbulent Molecular Clouds II - from 0.1 to 0.01 parsec
• High Resolution CO Observations of Massive Star Forming Regions
• 870 Micron Dust Continuum of the Youngest Protostars in Ophiuchus
• Automated approach to measure stellar inclinations: validation through large-scale measurements on the red giant branch
• Gravitational instability and star formation in NGC 628
• A binary system in the S cluster close to the supermassive black hole Sagittarius A*
• The effects of ionization feedback on star formation: A case study of the M16 H II region
• Resolved Star Formation Efficiency in the Antennae Galaxies
• The magnetic properties of the protostellar core IRAS 15398-3359
• The interstellar medium and the massive stellar content toward the SNR G18.1-0.1 and neighboring HII regions
• Instability of Evaporation Fronts in the Interstellar Medium
• Gravitational instability of filamentary molecular clouds, including ambipolar diffusion
• Near-Infrared Imaging Polarimetry toward M17 SWex
• Dense Cloud Formation and Star Formation in a Barred Galaxy
• Kinematic classification of non-interacting spiral galaxies
• Impact of magnetic fields on Population III star formation
• Centroid Velocity Statistics of Molecular Clouds
• Ongoing hierarchical massive cluster assembly: the LISCA II structure in the Perseus complex
• The Catalogue for Astrophysical Turbulence Simulations (CATS)
• A multi-transition methanol maser study of the accretion burst source G358.93-0.03-MM1
• The Magnetic Field in the Milky Way Filamentary Bone G47
• A molecular outflow evidencing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
• Protostellar collapse: rotation and disk formation
• Testing the Evolutionary Sequence of High Mass Protostars with CARMA
• The Gaia-ESO Survey: N-body modelling of the Gamma Velorum cluster
• The Bolocam Galactic Plane Survey. XIII. Physical Properties and Mass Functions of Dense Molecular Cloud Structures
• Testing Magnetic Field Models for the Class 0 Protostar L1527
• Relative Alignment between Dense Molecular Cores and Ambient Magnetic Field: The Synergy of Numerical Models and Observations
• Magnetohydrodynamic turbulence in a strongly magnetised plasma
• The action principle for generalized fluid motion including gyroviscosity
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• Lecture notes on black hole binary astrophysics
• Instrumental performance and results from testing of the BLAST-TNG receiver, submillimeter optics, and MKID arrays
• Methods for compressible fluid simulation on GPUs using high-order finite differences
• Tracing Magnetic Field with Synchrotron Polarization Gradients: Parameter Study
• Fast deuterium fractionation in magnetized and turbulent filaments
• A comparison of shock-cloud and wind-cloud interactions: The longer survival of clouds in winds
• High-mass star formation in Orion possibly triggered by cloud-cloud collision III, NGC2068 and NGC2071
• Projected velocity statistics of interstellar turbulence
• Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud
• Tracing magnetic fields by the synergies of synchrotron emission gradients
• The structure of molecular gas associated with NGC2264: wide-field 12CO and H2 imaging
• Atomic and molecular gas properties during cloud formation
• Sub-kpc star-formation law in the local luminous infrared galaxy IC 4687 as seen by ALMA
• z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [III] Physical properties
• The Balloon-borne Large-Aperture Submillimeter Telescope for Polarization: BLAST-pol
• A thin diffuse component of the Galactic Ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries
• Lurking systematics in predicting galaxy cold gas masses using dust luminosities and star formation rates
• High-mass star formation at high luminosities: W31 at >10^6 L_sun
• Evidence for Decay of Turbulence by MHD Shocks in Molecular Clouds via CO Emission
• An ALMA study of outflow parameters of protoclusters: outflow feedback to maintain the turbulence
• The Shapes of Molecular Cloud Cores in Simulations and Observations
• Reconnection in weakly stochastic B-fields in 2D
• Signature of non-isotropic distribution of stellar rotation inclination angles in the Praesepe cluster
• On the Habitability of Universes without Stable Deuterium
• The spectrum of magnetized turbulence in the interstellar medium
• Light element variations in globular clusters via nucleosynthesis in black hole accretion discs
• An ALMA Glimpse of Dense Molecular Filaments Associated with High-mass Protostellar Systems in the Large Magellanic Cloud
• A Parsec-Scale Catalog of Molecular Clouds in the Solar Neighborhood Based on 3D Dust Mapping: Implications for the Mass-Size Relation
• Intensity-Corrected Herschel Observations of Nearby Isolated Low-Mass Clouds
• An Exploration of the Statistical Signatures of Stellar Feedback
• Distortion of Magnetic Fields in a Starless Core IV: Magnetic Field Scaling on Density and Mass-to-flux Ratio Distribution in FeSt 1-457
• Mid-infrared interferometry of the massive young stellar object NGC3603 - IRS 9A
• Transport of Protostellar Cosmic Rays in Turbulent Dense Cores
• The Probability Distribution Function of Gas Surface Density in M33
• Probing the clumping structure of Giant Molecular Clouds through the spectrum, polarisation and morphology of X-ray Reflection Nebulae
• Early Planet Formation in Embedded Disks (eDisk) IX: High-resolution ALMA Observations of the Class 0 Protostar R CrA IRS5N and its surrounding
• Probability distribution functions of gas in M31 and M51
• Binary Disk interaction II: Gap-Opening criteria for unequal mass binaries
• Precession and polar alignment of accretion discs in triple (or multiple) stellar systems
• Unveiling Extragalactic Star Formation Using Radio Recombination Lines: An EVLA Pilot Study with NGC 253
• HI Clouds in LITTLE THINGS Dwarf Irregular Galaxies
• The role of turbulence, magnetic fields and feedback for star formation
• The driving mode of shock-driven turbulence
• First-generation Science Cases for Ground-based Terahertz Telescopes
• Studying the local magnetic field and anisotropy of magnetic turbulence by synchrotron polarization derivative
• Magnetic fields in early protostellar disk formation
• Anomalous compressible mode generation by global frame projections of pure Alfven mode
• The Magnetized Environment of the W3(H2O) Protostars
• A Coordinated X-ray and Optical Campaign of the Nearby Massive Binary $\delta$ Orionis Aa: II. X-ray Variability
• A Kennicutt-Schmidt relation at molecular cloud scales and beyond
• Modeling the physical properties in the ISM of the low-metallicity galaxy NGC4214
• Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds. II. Directly Probing the Ion-neutral Decoupling Scale
• Starless Cloud Core L1517B in Envelope Expansion with Core Collapse
• Unveiling molecular clouds toward bipolar HII region G8.14+0.23
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Triggered massive star formation associated with the bubble HII region Sh2-39 (N5)
• Formation and evolution of the water maser outflow event in AFGL 2591 VLA 3-N
• An Extension of the Athena++ Framework for Fully Conservative Self-Gravitating Hydrodynamics
• The early dynamical evolution of star clusters near the Galactic Centre
• The interaction of a magnetohydrodynamical shock with a filament
• On the accretion process in a high-mass star forming region - A multitransitional THz Herschel-HIFI study of ammonia toward G34.26+0.15
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• Comparison of Prestellar Core Elongations and Large-Scale Molecular Cloud Structures in the Lupus I Region
• New constraints on the physical conditions in H${}_2$-bearing GRB-host damped Lyman-$\alpha$ absorbers
• Denoising Diffusion Probabilistic Models to Predict the Density of Molecular Clouds
• Mapping the Galactic Magnetic Field Orientation and Strength in Three Dimensions
• Transition from ordered pinched to warped magnetic field on a 100 au scale in the Class 0 protostar B335
• CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
• Two modes of carbonaceous dust alignment
• Probing Three-Dimensional Magnetic Fields: I -- Polarized Dust Emission
• Application of Convolutional Neural Networks to Identify Protostellar Outflows in CO Emission
• Polarised emission from aligned dust grains in nearby galaxies: predictions from the Auriga simulations
• A Significant Population of Candidate New Members of the Rho Ophiuchi Cluster
• The "Maggie" filament: Physical properties of a giant atomic cloud
• Two-Stage Fragmentation for Cluster Formation: Analytical Model and Observational Considerations
• Dynamical dust traps in misaligned circumbinary discs: analytical theory and numerical simulations
• Centrifugal barriers in magnetospheric accretion
• Advanced Diagnostics for the Study of Linearly Polarized Emission. II: Application to Diffuse Interstellar Radio Synchrotron Emission
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement
• Star Formation Activity in the Long, Filamentary Infrared Dark Cloud G53.2
• Hierarchical star formation in nearby galaxies
• Understanding the Geometry of Astrophysical Magnetic Fields
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• Induced Core Formation Time in Subcritical Magnetic Clouds by Large-Scale Trans-Alfvénic Flows
• Spatial variations of turbulent properties of neutral hydrogen gas in the Small Magellanic Cloud using structure function analysis
• Physical characteristics of G331.5-0.1: The luminous central region of a Giant Molecular Cloud
• The Astrophysical Environment of the Solar Birthplace
• Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
• Clumps as multiscale structures in cosmic noon galaxies
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds III: SLED fitting
• The inflow signature toward different evolutionary phases of massive star formation
• Class I methanol masers in low-mass star formation regions
• A comparison of shock-cloud and wind-cloud interactions: effect of increased cloud density contrast on cloud evolution
• The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
• Evolution of Magnetic Fields in Collapsing Star-forming Clouds under Different Environments
• Evolutionary tracks of massive stars during formation
• Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics?
• A new method for probing magnetic field strengths from striations in the interstellar medium
• Multi-Phase Magnetic Fields in the Galaxy NGC 3627
• On-Sky Demonstration of a Linear Band-limited Mask with Application to Visual Binary Stars
• Opacity Broadening of ${}^{13}$CO Linewidths and its Effect on the Variance-Sonic Mach Number Relation
• WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
• Numerical viscosity and resistivity in MHD turbulence simulations
• Searching for Inflow Towards Massive Starless Clump Candidates Identified in the Bolocam Galactic Plane Survey
• Which Part of Dense Cores Feeds Material to Protostars?: The Case of L1489 IRS
• The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina
• Velocity Anisotropy in Self-Gravitating Molecular Clouds. I: Simulation
• Curved jet motion. I. Orbiting and precessing jets
• ALMA Observations of Giant Molecular Clouds in M33. II. Triggered High-mass Star Formation by Multiple Gas Colliding Events at the NGC 604 Complex
• Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
• Diagnosis of 3D magnetic field and modes composition in MHD turbulence with Y-parameter
• A comparison between Faraday Tomography and Synchrotron Polarization Gradients
• The alignment is in their stars: on the spin-alignment of stars in star clusters
• Effect of lithium hydride on the cooling of primordial gas
• Star Cluster Formation from Turbulent Clumps. I. The Fast Formation Limit
• The nature of very low luminosity objects (VeLLOs)
• A Study of Stellar Spins in 15 Open Clusters
• Membership analysis and 3D kinematics of the star-forming complex around Trumpler 37 using Gaia-DR3
• Wide binary stars formed in the turbulent interstellar medium
• Cluster formation in molecular clouds: I. stellar populations, star formation rates, and ionizing radiation
• A statistical measurement of the HI spin temperature in DLAs at cosmological distances
• The effect of diffuse background on the spatially-resolved Schmidt relation in nearby spiral galaxies
• Studying Anisotropy of Compressible Magnetohydrodynamic Turbulence by Synchrotron Polarization Intensity
• The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks
• MHD simulations of the formation and propagation of protostellar jets to observational length scales
• On the nature of the enigmatic object IRAS 19312+1950: A rare phase of massive star formation?
• Long-lived Magnetic-Tension-Driven Modes in a Molecular Cloud
• Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity
• Magnetic Field Structure of the HH 1-2 Region: Near-Infrared Polarimetry of Point-Like Sources
• Structures in circumbinary disks: Prospects for observability
• Emergence of the Kennicutt-Schmidt Relation from the Small-Scale SFR-Density Relation
• First Light II: Emission Line Extinction, Population III Stars, and X-ray Binaries
• The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry-BLASTPol: Performance and results from the 2012 Antarctic flight
• Extended Scaling Laws in Numerical Simulations of MHD Turbulence
• A comparison of the Milky Way's recent star formation revealed by dust thermal emission and high-mass stars
• Polarimetric and photometric investigation of a dark globule LDN 1225: distance, extinction law, and magnetic fields
• Role of Electon Excitation and Nature of Molecular Gas in Cluster Central Elliptical Galaxies
• On the distribution of the Cold Neutral Medium in galaxy discs
• A multi-frequency study of sub-parsec jets with the Event Horizon Telescope
• IRAS16547-4247: A New Candidate of a Protocluster Unveiled with ALMA
• Deconstructing the High-Mass Star-Forming Region IRAS 23033+5951
• Thermal design and performance of the balloon-borne large aperture submillimeter telescope for polarimetry BLASTPol
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds I
• Morphology of prestellar cores in pressure confined filaments
• Gravitational Instability of Rotating, Pressure-Confined, Polytropic Gas Disks With Vertical Stratification
• A very young, compact bipolar H${}_2$O maser outflow in the intermediate-mass star-forming LkH$\alpha$ 234 region
• Clusters, Clouds, and Correlations: Relating Young Clusters to Giant Molecular Clouds in M33 and M31
• Evolution of the Hub-filament Structures in IC 5146 in the Context of the Energy Balance of Gravity, Turbulence, and Magnetic Field
• On the frequencies of circumbinary discs in protostellar systems
• A physically motivated `charge-exchange method' for measuring electron temperatures within HII regions
• Resolution-dependent Subsonic Non-thermal Line Dispersion Revealed by ALMA
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• The complete census of molecular hydrogen in a simulated disc galaxy
• Molecular gas toward the Gemini OB1 Giant Molecular Cloud Complex I: Observation data
• Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC7674
• Coupling local to global star formation in spiral galaxies: the effect of differential rotation
• Modelling the structure of molecular clouds: I. A multi-scale energy equipartition
• Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification
• ALMA-IMF XVI: Mass-averaged temperature of cores and protostellar luminosities in the ALMA-IMF protoclusters
• Magnetohydrodynamics with GAMER
• A turbulent origin for the complex envelope kinematics in the young low-mass core Per-Bolo 58
• On the evolution of the observed Mass-to-Length relationship for star-forming filaments
• Magnetic Field Structure in Spheroidal Star-Forming Clouds. II. Estimating Field Structure from Observed Maps
• Alignment of dense molecular core morphology and velocity gradients with ambient magnetic fields
• Principal Component Analysis studies of turbulence in optically thick gas
• Bow Magnetic Morphology Surrounding Filamentary Molecular Clouds? 3D Magnetic Field Structure of Orion-A
• Supersonic turbulence in 3D isothermal flow collision
• Description of turbulent dynamics in the interstellar medium: multifractal/microcanonical analysis I. Application to Herschel observations of the Musca filament
• Turbulence decay and cloud core relaxation in molecular clouds
• Infall, outflow, and turbulence in massive star-forming cores in the G333 giant molecular cloud
• Testing the global star formation relation: An HCO+ (3-2) mapping study of Red MSX sources in the Bolocam Galactic Plane Survey
• Polar alignment of a massive retrograde circumbinary disc around an eccentric binary
• Molecular tracers of radiative feedback in Orion (OMC-1). Widespread CH+ (J=1-0), CO (10-9), HCN (6-5), and HCO+ (6-5) emission
• Ion and neutral molecules in the W43-MM1(G30.79 FIR 10) infalling clump
• Velocity centroid gradients for absorbing media
• Physics of Non-Universal Larson's Relation
• The Role of Non-ionizing Radiation Pressure in Star Formation: The Stability of Cores and Filaments
• The Closest M-Dwarf Quadruple System to the Sun
• Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence
• Star Formation Variability as a Probe for the Baryon Cycle within Galaxies
• An APEX survey of outflow and infall toward the youngest protostars in Orion
• Evolution of the atomic component in protostellar outflows
• Dependence of the Star Formation Efficiency on the Parameters of Molecular Cloud Formation Simulations
• A Tale of 3 Dwarfs: No Extreme Cluster Formation in Extreme Star-Forming Galaxies
• Star-forming regions of the Aquila rift cloud complex. II. Turbulence in molecular cores probed by NH3 emission
• Nobeyama 45-m Mapping Observations toward Orion A. III. Multi-Line Observations toward an Outflow-shocked Region, OMC-2 FIR
• High-resolution APEX/LAsMA ${}^{12}$CO and ${}^{13}$CO (3-2) observation of the G333 giant molecular cloud complex : II. Survival and gravitational collapse of dense gas structures under feedback
• The Evolution of Molecular Gas Fraction Traced by the CO Tully-Fisher Relation
• Dissociative Recombination of Rotationally Cold OH${}^{+}$ and Its Implications for the Cosmic Ray Ionization Rate in Diffuse Clouds
• The hydrodynamical models of the cometary compact H II region
• JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H${}_2$ in the radio galaxy 3C 326 N
• Characterising the Magnetic Fields of Nearby Molecular Clouds using Submillimeter Polarization Observations
• Magnetic field geometry of the large globule CB 34
• Intermittency of Fast MHD Modes and Regions of Anomalous Gradient Orientation in Low-beta Plasmas
• Magnetic Field Strengths in Photodissociation Regions
• The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
• Protostar L1455 IRS1: Rotating Disk Connecting to Filamentary Network
• Theoretical modelling of two-component molecular discs in spiral galaxies
• Near-IR imaging towards a puzzling YSO precessing jet
• The tight correlation of PAH and CO emission from z~0-4
• Observations and radiative transfer modelling of a massive dense cold core in G333
• Resolved star formation in the metal poor star-forming region Magellanic Bridge C
• Internal Structure of the Jets from Young Stars Simulated at Plasma Focus Facilities
• Unveiling the role of galactic rotation on star formation
• The Molecular Gas Environment around Two Herbig Ae/Be Stars: Resolving the Outflows of LkHa 198 and LkHa 225S
• Molecular gas budget and characterization of intermediate-mass star-forming galaxies at $z\approx 2-3$
• Distortion of Magnetic Fields in a Starless Core VI: Application of Flux Freezing Model and Core Formation of FeSt 1-457
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Characterization of Turbulence from Submillimeter Dust Emission
• Exploring morphological correlations among H2CO, 12CO, MSX and continuum mappings
• Spokes cluster: The search for the quiescent gas
• Structure of CB 26 Protoplanetary Disk Derived from Millimeter Dust Continuum Maps
• Gravity or turbulence V: Star forming regions undergoing violent relaxation
• The disk-outflow system around the rare young O-type protostar W42-MME
• A Synergy of the Velocity Gradients Technique and the Probability Density Functions for Identifying Gravitational Collapse in Self-Absorbing Media
• Generation of Solenoidal Modes and Magnetic Fields in Turbulence Driven by Compressive Driving
• Cloud properties across spatial scales in simulations of the interstellar medium
• The Column Density Structure of Orion A Depicted by N-PDF
• A mapping study of L1174 with 13CO J=2-1 and 12CO J=3-2: star formation triggered by a Herbig Ae/Be star
• Molecular Clouds: Internal Properties, Turbulence, Star Formation and Feedback
• The Equilibrium Structure of Prolate Magnetized Molecular Cores
• Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
• Modifying two-body relaxation in N-body systems by gas accretion
• Radiation feedback in dusty clouds
• Magnetic fields and Star Formation around HII regions: The S235 complex
• Structure analysis of simulated molecular clouds with the Delta-variance
• Magnetic fields in gaps surrounding giant protoplanets
• Modeling Turbulence in Galactic Centers
• Census of Gaseous Satellites around Local Spiral Galaxies
• Magnetic Field in The Isolated Massive Dense Clump IRAS 20126+4104
• Magnetic Field of Molecular Gas Measured with the Velocity Gradient Technique I. Orion A
• The physical state of selected cold clumps
• Magnetic Flux Transport by turbulent reconnection in astrophysical flows
• Consequences of cosmic microwave background-regulated star formation
• Spectroscopic Confirmation of a Population of Isolated, Intermediate-Mass YSOs
• Exploring Galactic open clusters with Gaia I. An examination in the first kiloparsec
• Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
• Rankine-Hugoniot Relations in Relativistic Combustion Waves
• Extreme star formation in the Milky Way: Luminosity distributions of young stellar objects in W49A and W51
• First Star Formation in the Presence of Primordial Magnetic Fields
• Spritz is sparkling: simulated CO and [CII] luminosities
• Effects of Turbulence on Cosmic Ray Propagation in Protostars and Young Star/Disk Systems
• Formation of metal-free binaries: Impact of H${}_2$ line cooling and CIE cooling
• X-raying molecular clouds with a short flare: probing statistics of gas density and velocity fields
• Sub-kiloparsec empirical relations and excitation conditions of HCN and HCO+ J=3-2 in nearby star-forming galaxies
• Dust evolution during the protostellar collapse: influence on the coupling between the neutral gas and the magnetic field
• Application of Convolutional Neural Networks to Predict Magnetic Fields Directions in Turbulent Clouds
• A Unified Model for Bipolar Outflows from Young Stars: Apparent Magnetic Jet Acceleration
• Latest news on the Physics of Brown dwarfs
• A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia
• The Twisted Magnetic Field of the Protobinary L483
• Driving Conditions of Protostellar Outflows in Different Star-Forming Environments
• Extraplanar H II Regions in Spiral Galaxies. II. In Situ Star Formation in the Interstellar Thick Disk of NGC 4013
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Outflow, Infall and Protostars in the Star Forming Core W3-SE
• Distortion of Magnetic Fields in a Starless Core V: Near-infrared and Submillimeter Polarization in FeSt 1-457
• Metallicity dependence of the CO-to-H${}_2$ and the [CI]-to-H${}_2$ conversion factors in galaxies
• Constraints on galactic wind models
• Young Stellar Object candidates toward the Orion region selected from GALEX
• The ionization fraction in OMC-2 and OMC-3
• The Mid-Infrared Polarization of the Herbig Ae Star WL 16: An Interstellar Origin?
• Herschel observations of the circumstellar environment of the two Herbig Be stars R Mon and PDS27
• The Star-Forming Interstellar Medium of Lyman Break Galaxy Analogs
• Sagittarius B2 Main: A Cluster of Ultra-Compact HII Regions and Massive Protostellar Cores
• Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE. The diverse ionization mechanisms acting in low-mass starbursts
• The Dependence of Prestellar Core Mass Distributions on the Structure of the Parental Cloud
• Characterization of dense Planck clumps observed with Herschel and SCUBA-2
• Feedback in Forming Star Clusters: The Mass-Radius Relation and Mass Function of Molecular Clumps in the Large Magellanic Cloud
• Nobeyama 45 m Local Spur CO survey. I. Giant molecular filaments and cluster formation in the Vulpecula OB association
• A${}^3$COSMOS: the dust mass function and dust mass density at $0.5<z<6$
• Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds
• Aligned grains and inferred toroidal magnetic fields in the envelopes of massive young stellar objects
• High-Mass Starless Clumps: Dynamical State and Correlation Between Physical Parameters
• Testing assumptions and predictions of star-formation theories
• CRAFT (Cosmic Ray Acceleration From Turbulence) in Molecular Clouds
• Core orientations and magnetic fields in isolated molecular clouds
• Physical Properties and Scaling Relations of Molecular Clouds: the Impact of Star Formation
• High-sensitivity millimeter imaging of molecular outflows in nine nearby high-mass star-forming regions
• Low-Mass Star Forming Cores in the GF9 Filament
• Neutral hydrogen filaments in interstellar media: Are they physical?
• Illuminating a tadpole's metamorphosis II: observing the on-going transformation with ALMA
• On recent SFR calibrations and the constant SFR approximation
• Molecular Line Ratio Diagnostics Along the Radial Cut and Dusty UV-bright Clumps in a Spiral Galaxy NGC 0628
• The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
• An extended hybrid numerical simulation of isotropic compressible turbulence
• Evidence of interacting elongated filaments in the star-forming site AFGL 5142
• Gravitational instability of filamentary molecular clouds, including ambipolar diffusion; Non-isothermal filament
• Gravitationally Bound Gas Determines Star Formation in the Galaxy
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• A Tale of Two Clump Masses: A New Way to Study Clump Formation in Simulations
• Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei
• Relative alignment between gas structures and magnetic field in Orion A at different scales using different molecular gas tracers
• Turbulent magnetic field in the HII region Sh 2-27
• HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
• The Cassiopeia Filament: A Blown Spur of the Local Arm
• Nobeyama Survey of Inward Motions toward Cores in Orion Identified by SCUBA-2
• Infrared study of the star-forming region associated with the UC HII regions G45.07+0.13 and G45.12+0.13
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• The Astrochemical Evolution of Turbulent Giant Molecular Clouds : I - Physical Processes and Method of Solution for Hydrodynamic, Embedded Starless Clouds
• Mapping and characterizing magnetic fields in the Rho Ophiuchus-A molecular cloud with SOFIA/HAWC$+$
• DIISC-II: Unveiling the Connections between Star Formation and ISM in the Extended Ultraviolet Disk of NGC 3344
• Clustering of low mass stars around Herbig Be star IL Cep -- Evidence of "Rocket Effect" using Gaia EDR3 ?
• The Transition of Polarized Dust Thermal Emission from the Protostellar Envelope to the Disk Scale
• Saturation level of turbulence in collapsing gas clouds
• Dense gas and exciting sources of the molecular outflow in the AFGL 437 star-forming region
• CO Outflow Candidates Toward the W3/4/5 Complex II: Feedback from Candidate Outflows
• Photoionization feedback in turbulent molecular clouds
• Gradient measurement of synchrotron polarization diagnostic: Application to spatially separated emission and Faraday rotation regions
• Cosmic Ray transport in turbulent magnetic field
• A Mystery in Chamaeleon: Serendipitous Discovery of a Galactic Symbiotic Nova
• Effects of the magnetic field direction on the Tsallis statistic
• Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS
• A Model for Protostellar Cluster Luminosities and the Impact on the CO-H${}_2$ Conversion Factor
• Proper Motions of Young Stellar Outflows in the Mid-Infrared with Spitzer. II. HH 377/Cep E
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Cloud-cloud collision and star formation in G013.313+0.193
• Energy Transfer and Spectra in Simulations of Two-dimensional Compressible Turbulence
• Resistive Heating Induced by Streaming Cosmic Rays Around a Galaxy in the Early Universe
• Spectroscopic infrared extinction mapping as a probe of grain growth in IRDCs
• Comparison of Two Epochs of the Zeeman Effect in the 44 GHz Class I methanol (CH3OH) maser line in OMC-2
• The Environments of CO Cores and Star Formation in the Dwarf Irregular Galaxy WLM
• The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"
• Submillimeter Array CO(2-1) Imaging of the NGC 6946 Giant Molecular Clouds
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XVII. Statistical properties of individual HII regions in unperturbed systems
• A sensitive, high-resolution, wide-field IRAM NOEMA CO(1-0) survey of the very nearby spiral galaxy IC 342
• The BLAST Survey of the Vela Molecular Cloud: Dynamical Properties of the Dense Cores in Vela-D
• Energy conserving and well-balanced discontinuous Galerkin methods for the Euler-Poisson equations in spherical symmetry
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Long-Term Evolution of Decaying MHD Turbulence in the Multiphase ISM
• On the role of magnetic fields in star formation
• Fragmentation and Evolution of Molecular Clouds. III: The Effect of Dust and Gas Energetics
• Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
• SCOTCH -- Search for Clandestine Optically Thick Compact HIIs
• New method for estimating molecular cloud distances based on Gaia, 2MASS, and the TRILEGAL galaxy model
• A Giant Molecular Cloud Catalog in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
• Observing with NIKA2Pol from the IRAM 30m telescope. Early results on the commissioning phase
• Statistical properties and correlation length in star-forming molecular clouds: I. Formalism and application to observations
• Laboratory Photoionization Fronts in Nitrogen Gas: A Numerical Feasibility and Parameter Study
• Kinematics of Subclusters in Star Cluster Complexes: Imprint of their Parental Molecular Clouds
• Spectroscopic Evidence for Gas Infall in GF9-2
• Multi log-normal density structure in Cygnus-X molecular clouds: A fitting for N-PDF without power-law
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• SOFIA and ALMA Investigate Magnetic Fields and Gas Structures in Massive Star Formation: The Case of the Masquerading Monster in BYF 73
• ALMA Observations for CO Emission from Luminous Lyman-break Galaxies at $z=6.0293$-$6.2037$
• The first detection of cosmic-ray excited H${}_2$ in interstellar space
• Chemical and Physical Conditions in Molecular Cloud Core DC 000.4-19.5 (SL42) in Corona Australis
• On the Coagulation and Size Distribution of Pressure Confined Cores
• Searching for converging flows of atomic gas onto a molecular cloud
• Magnetic field measurement from the Davis-Chandrasekhar-Fermi method employed with Atomic Alignment
• A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
• Testing Models of Triggered Star Formation with Young Stellar Objects in Cepheus OB4
• High-Resolution M-band Spectroscopy of CO towards the Massive Young Stellar Binary W3 IRS5
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• Cosmic Ray Feedback on Bi-stable ISM Turbulence
• When the Stars Align: A 5 σ Concordance of Planetary Nebulae Major Axes in the Centre of our Galaxy
• Generation of high circular polarization of interstellar Lyman $\alpha$ radiation triggering biological homochirality
• Atomic Modeling of Photoionization Fronts in Nitrogen Gas
• Discovery of a New Molecular Bubble-Outflow Structure in the Taurus B18 Cloud
• Bimodal Star Formation in Simulations of Strongly Magnetized Giant Molecular Clouds
• Formation of Transient High-$\beta$ Plasmas in a Magnetized, Weakly Collisional Regime
• Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
• The long-term evolution of main-sequence binaries in DRAGON simulations
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
• Giant Cometary HII Regions and Molecular Bow Shocks in Spiral Arms of Galaxies: M83
• Detecting episodes of star formation using Bayesian model selection
• Prestellar Cores in Turbulent Clouds: Numerical Modeling and Evolution to Collapse
• Growth problems of stellar black holes in early galaxies
• A rotating helical filament in the L1251 dark cloud
• Probing the Physics of Star-Formation (ProPStar) III. No evidence for dissipation of turbulence down to 20 mpc (4 000 au) scale
• A self-gravity module for the PLUTO code
• Searching for further evidence for cloud-cloud collisions in L1188
• Metal Enrichment and Reionization Constraints on Early Star Formation
• Molecular Bow Shock in the 3-kpc Norma Arm
• Spherically-symmetric, cold collapse: the exact solutions and a comparison with self-similar solutions
• Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
• The G 305 Star-forming Region: II. Irregular variable stars
• Prograde spin-up during gravitational collapse
• Miec: A Bayesian hierarchical model for the analysis of nearby young open clusters
• Turbulence and its connection to episodic accretion in binary YSOs
• Tracing the Formation of Molecular Clouds in a Low-Metallicity Galaxy: A HI Narrow Self-Absorption Survey of the Large Magellanic Cloud
• Don't torque like that. Measuring compact object magnetic fields with analytic torque models
• The warm and dense Galaxy - tracing the formation of dense cloud structures out to the Galactic Center
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• Star formation drivers across the M33 disk
• Detection of molecular clouds in the PeVatron candidate source LHAASO J0341$+$5258 by the Nobeyama 45-m radio telescope
• Formation of low-mass stars and brown dwarfs
• A Deep Neural Network Approach to Compact Source Removal
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• The Luminosity Problem: Testing Theories of Star Formation
• Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
• Probing the physical and chemical structure of the CS core in LDN 673. Multitransitional and continuum observations
• Massive star cluster formation III. Early mass segregation during cluster assembly
• Studying Interstellar Turbulence Driving Scales using the Bispectrum
• Post-Newtonian corrections to Toomre's criterion
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Imaging polarimetry of the rotating Bok globule CB67
• Turbulence driven by stellar jets, the possibility and the efficiency
• Relative Alignment Between Magnetic Fields and Molecular Gas Structure in Molecular Clouds
• Unveiling the initial conditions of open star cluster formation
• The Correlation of Dust and Gas Emission in Star-Forming Environments
• Faraday Rotation Distributions from Stellar Magnetism in Wind-Blown Bubbles
• The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
• The Young Stellar Population, Distance, and Cloud-Cloud Collision Induced Star Formation Scenario of the Trifid Nebula
• A Statistical Study of H I Gas in Nearby Narrow-Line AGN-Hosting Galaxies
• Touching the Stars: Using High-Resolution 3D Printing to Visualize Stellar Nurseries
• ALMA ${}^{13}\mathrm{CO}$(J=1-0) Observations of NGC 604 in M33: Physical Properties of Molecular Clouds
• Pre main sequence: Accretion & Outflows
• Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences
• Ambipolar diffusion: Self-similar solutions and MHD code testing. Cylindrical symmetry
• Widespread subsonic turbulence in Ophiuchus North 1
• Focusing MHD Wave as a Trigger of Star Formation
• Magnetic fields of Herbig Ae/Be stars
• Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations
• Northern Galactic Molecular Cloud Clumps in Hi-GAL: Clump and Star Formation within Clouds
• A High-Mass Young Star-forming Core Escaping from Its Parental Filament
• Massive Young Stellar Objects and Outflow in the Infrared-Dark Cloud G79.3+0.3
• Non-similar collapse of singular isothermal spherical molecular cloud cores with nonzero initial velocities
• Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
• Optical polarimetry study of Lambda-Orionis star-forming region
• Density profile of a self-gravitating polytropic turbulent fluid in a rotating disk near to the cloud core
• Prestellar Cores in Turbulent Clouds: Properties of Critical Cores
• ArTéMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps
• Local Stability of Galactic Discs in Modified Dynamics
• On the shape of the mass-function of dense clumps in the Hi-GAL fields. II. Using Bayesian inference to study the clump mass function
• A Galactic Molecular Cloud Clump Catalog from Hi-GAL Data: Method and Initial Results Comparison to BGPS
• Matter Infall in Collapsing Molecular Cloud Cores with an Axial Magnetic Field
• Studying the properties of compressible MHD turbulence by synchrotron fluctuation statistics
• Linear stability of a rotating liquid column revisited
• The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
• Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions
• Dynamical evolution of the open clusters with different star formation efficiencies and orbital parameters
• Diagnostics of magnetohydrodynamic modes in the ISM through synchrotron polarization statistics
• MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations
• Characterising the physical and chemical properties of a young Class 0 protostellar core embedded in the Orion B9 filament
• Tree-based solvers for adaptive mesh refinement code FLASH -- IV: An X-ray radiation scheme to couple discrete and diffuse X-ray emission sources to the thermochemistry of the interstellar medium
• A Catalog of Stellar and Dust Properties for 500,000 Stars in the Southwest Bar of the Small Magellanic Cloud
• The Drag Instability in a 1D Isothermal C-Shock
• Deuterium fractionation of the starless core L 1498
• Super-Eddington Growth Ceiling: Analytic Constraints on the Rapid Growth of Light-Seed Black Holes in Massive Clumps
• Wavelength-dependent far-infrared polarization of HL Tau observed with SOFIA/HAWC+
• Evidence for protostellar jets as a population of hadronic gamma-ray sources
• The Sharpest Ultraviolet view of the star formation in an extreme environment of the nearest Jellyfish Galaxy IC 3418
• Simulations of the IMF in Clusters
• The superclouds of the local Milky Way
• On the Interaction between Turbulence and a Planar Rarefaction
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• The Star Formation Relation in Nearby Galaxies
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Detection of Dust Condensations in the Orion Bar Photon-dominated Region
• Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
• Cloud structure and young star distribution in the Dragonfish complex
• The kinematics of the magnetised protostellar core IRAS15398-3359
• Obtaining strength of magnetic field from E and B modes of dust polarization
• Natal molecular cloud of SNR Kes 41. Complete characterisation
• Comparing the morphology of molecular clouds without supervision
• The JCMT Nearby Galaxies Legacy Survey: SCUBA-2 observations of nearby galaxies
• Disk-outflow models as applied to high mass star forming regions through methanol and water maser observations
• Clumpy shocks as the driver of velocity dispersion in molecular clouds: the effects of self-gravity and magnetic fields
• Experimental and Numerical Studies of the Collapse of Dense Clouds Induced by Herbig-Haro Stellar Jets
• Modeling Local Bubble analogs II: Synthetic Faraday rotation maps
• Structure of iso-density sets in supersonic isothermal turbulence
• New constraints on the initial parameters of low-mass star formation from chemical modeling
• Constraints on the collimated X-ray emission of SS 433 from the reflection on molecular clouds
• Dust and Gas environment of the young embedded cluster IRAS 18511+0146
• The Warm-Hot Disk-Halo Interface Below the Perseus Spiral Arm
• MHD turbulence-Star Formation Connection: from pc to kpc scales
• Tiny-Scale Properties within the Interstellar Medium towards PSR J1644$-$4559: I. Observational Evidence of Turbulence-induced Tiny Scale Atomic Structures
• From Stellar Nurseries to Old Stellar Populations: A Multi-wavelength Case of NGC 1055
• Cloud fragmentation cascades and feedback: on reconciling an unfettered inertial range with a low star formation rate
• The first stars
• Sapaki: Galactic O3If* star possibly born in isolation
• Bridging Theory and Observation: Synthetic Far-infrared Insights into Star Formation Efficiency
• HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
• Population I Cepheids and understanding star formation history of the Small Magellanic Cloud
• Dense clumps survive in the vicinity of R136 in 30 Doradus
• Centrally concentrated star formation in young clusters
• Tight correlation of star formation with [Ci] and CO lines across cosmic time
• Fire from Ice - Massive Star Birth from Infrared Dark Clouds
• Near-Infrared Photometry and Radio Continuum Study of the Massive Star Forming Regions IRAS 21413+5442 and IRAS 21407+5441
• Parallel and Perpendicular Alignments of Velocity Gradient and Magnetic Field observed in the Molecular Clouds L1478 and L1482
• Thermal damping of Weak Magnetosonic Turbulence in the Interstellar Medium
• Statistical properties and correlation length in star-forming molecular clouds: II. Gravitational potential and virial parameter
• Telescopes versus Microscopes: the puzzle of Iron-60
• Prospects of Turbulence Studies in High-Energy Density Laser-Generated Plasma: Numerical Investigations in Two Dimensions
• When did the initial mass function become bottom-heavy?
• QPO-Based Bayesian Constraints on Charged Particle Dynamics Around Magnetized Schwarzschild Black Holes
• Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
• Molecular cloud matching in CO and dust in M33 II. Physical properties of giant molecular clouds
• Star Formation and Gas Dynamics in Galactic Disks: Physical Processes and Numerical Models
• Unveiling the evolution of the CO excitation ladder through cross-correlation of CONCERTO-like experiments and galaxy redshift surveys
• Ancillary science with Ariel: Feasibility and scientific potential of young stellar object observations
• Galaxy Activity, Torus and Outflow Survey (GATOS) X: Molecular gas clumpiness under the influence of AGN
• Laboratory Modeling of Supernova Remnants Collisions: Implications for Triggered Star Formation
• Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
• Magnetic clumping of charged dust in the dense interstellar medium
• Collapsing Index: A New Method to Identify Star-forming Cores Based on ALMA Images
• Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
• Alfven number for the Richtmyer-Meshkov instability in magnetized plasmas
• Study of a Population of Gamma-ray Bursts with Low-Luminosity Afterglows
• Neutral Stellar Winds Toward the High-Mass Star-Forming Region G176.51+00.20
• Effect of dust rotational disruption by radiative torques on radiation pressure feedback from massive protostars
• From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data
• Investigations of MWISP Bubbles: Identification and Analysis of Enclosed Molecular Bubbles by Weight Fields
• Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars
• A runaway T-Tauri star leaving an extended trail
• The interdependence between density PDF, CMF and IMF and their relation with Mach number in simulations
• Comparative study of the relationships between CO isotopic luminosities and infrared luminosity for the Galactic dense cores
• Shock fragmentation model for gravitational collapse
• Investigating the physical properties and fragmentation of the AFGL 333-Ridge
• Galactic cold cores II. Herschel study of the extended dust emission around the first Planck detections
• Why most molecular clouds are gravitationally dominated
• Modeling turbulent and self-gravitating fluids with Fourier neural operators
• SiO emission in the filamentary Infrared Dark Cloud G035.39-00.33: An ALMA view
• A Dynamic Galaxy: Stellar Age Patterns Across the Disk of M101
• Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations
• The signature of large scale turbulence driving on the structure of the interstellar medium
• Weak CS Emission in an Extremely Metal-poor Galaxy DDO 70
• A comprehensive catalogue of OB cluster candidates in M31 and their association with giant molecular clouds
• Turbulence Mode Decomposition and Anisotropy in Magnetically Dominated Collisionless Plasmas
• Magnetic Fields in Molecular Clouds -- Observation and Interpretation
• Intermittency and non-universality of pair dispersion in isothermal compressible turbulence
• Connecting the formation of stars and planets. II: coupling the angular momentum of stars with the angular momentum of planets
• Synthetic observations using POLARIS: an application to simulations of massive prestellar cores
• A Streamer Driving Misalignment in the Circumtriple Disk of GW Ori
• Non-ideal MHD and protostellar feedback effects on disc formation and evolution in numerical simulations of star cluster formation
• Stars throw their weight in old galaxies
• Explosive ejections generated by gravitational interactions
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies
• Sutra : An integrated framework for identification and characterization of filaments in the interstellar medium
• The road toward a full, high resolution Molecular Cloud catalog of the Galaxy
• Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes
• Interstellar medium and star formation studies with the Square Kilometre Array
• CO Structures with Narrow Lines in Nearby Quiescent Regions
• Young massive stars and their environment in the mid-infrared at high angular resolution
• The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics
• Density profile of a self-gravitating polytropic turbulent fluid in the context of ensembles of molecular clouds
• Near-Infrared Polarimetric Study of N159/N160 Star-Forming Complex in the Large Magellanic Cloud