Control of star formation by supersonic turbulence

Abstract

Understanding the formation of stars in galaxies is central to much of modern astrophysics. For several decades it has been thought that stellar birth is primarily controlled by the interplay between gravity and magnetostatic support, modulated by ambipolar diffusion. Recently, however, both observational and numerical work has begun to suggest that support by supersonic turbulence rather than magnetic fields controls star formation. In this review we outline a new theory of star formation relying on the control by turbulence. We demonstrate that although supersonic turbulence can provide global support, it nevertheless produces density enhancements that allow local collapse. Inefficient, isolated star formation is a hallmark of turbulent support, while efficient, clustered star formation occurs in its absence. The consequences of this theory are then explored for both local star formation and galactic scale star formation. (ABSTRACT ABBREVIATED)

Invited review for "Reviews of Modern Physics", 87 pages including 28 figures, in press

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• Baryon Cycles in the Biggest Galaxies
• Tracing magnetic fields with spectroscopic channel maps
• Gas dynamics in Massive Dense Cores in Cygnus-X
• Vertical Equilibrium, Energetics, and Star Formation Rates in Magnetized Galactic Disks Regulated by Momentum Feedback from Supernovae
• Radiation Feedback and Fragmentation in Massive Protostellar Cores
• The Virial Balance of Clumps and Cores in Molecular Clouds
• The density structure and star formation rate of non-isothermal polytropic turbulence
• The dynamics of collapsing cores and star formation
• The supernova-regulated ISM. I. The multi-phase structure
• Simulating Star Formation and Feedback in Galactic Disk Models
• Formation of Magnetized Prestellar Cores with Ambipolar Diffusion and Turbulence
• Accretion Outbursts in Self-gravitating Protoplanetary Disks
• Radial Profiles of Star Formation in the Far Outer Regions of Galaxy Disks
• A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence
• Is the Scaling of Supersonic Turbulence Universal?
• Scaling Relations of Star-Forming Regions: from kpc-size clumps to HII regions
• The Formation of the First Stars in the Universe
• The Field Condition: A New Constraint of Spatial Resolution in Simulations of the nonlinear Development of Thermal Instability
• A Simple and Accurate Network for Hydrogen and Carbon Chemistry in the ISM
• Maximally Star-Forming Galactic Disks II. Vertically-Resolved Hydrodynamic Simulations of Starburst Regulation
• The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds
• The modelling of feedback in star formation simulations
• Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• The SILCC project --- IV. Impact of dissociating and ionising radiation on the interstellar medium and Halpha emission as a tracer of the star formation rate
• Star formation in unbound giant molecular clouds: the origin of OB associations?
• A new density variance - Mach number relation for subsonic and supersonic, isothermal turbulence
• Optical polarimetry toward the Pipe nebula: Revealing the importance of the magnetic field
• Turbulence in the ICM from mergers, cool-core sloshing and jets: results from a new multi-scale filtering approach
• Simulations of the Milky Way's central molecular zone -- I. Gas dynamics
• The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
• Obtaining Spectra of Turbulent Velocity from Observations
• Robust HI kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario
• Properties of OB star-black hole systems derived from detailed binary evolution models
• Graph-based interpretation of the Molecular Interstellar Medium Segmentation
• The Galactic Center Cloud G0.253+0.016: A Massive Dense Cloud with low Star Formation Potential
• Stars with Photometrically Young Gaia Luminosities Around the Solar System (SPYGLASS) I: Mapping Young Stellar Structures and their Star Formation Histories
• Magnetic Fields in Diffuse H I and Molecular Clouds
• Dense Stellar Populations: Initial Conditions
• Magnetic Field Amplification by Small-Scale Dynamo Action: Dependence on Turbulence Models and Reynolds and Prandtl Numbers
• Generation of Magnetic Fields in the Multi-phase ISM with Supernova-Driven Turbulence
• Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse
• The structures of embedded clusters in the Perseus, Serpens and Ophiuchus molecular clouds
• A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces: I. Cloud-scale Gas Motions
• The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst
• On the Constancy of the Characteristic Mass of Young Stars
• An Excursion-Set Model for the Structure of GMCs and the ISM
• Non-linear diffusion of cosmic rays escaping from supernova remnants - I. The effect of neutrals
• Algorithmic comparisons of decaying, isothermal, supersonic turbulence
• Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
• An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• 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
• Molecular Cloud Evolution V. Cloud Destruction by Stellar Feedback
• Cholla : A New Massively-Parallel Hydrodynamics Code For Astrophysical Simulation
• The Turbulence Spectrum of Molecular Clouds in the Galactic Ring Survey: A Density-Dependent PCA Calibration
• Tsallis statistics as a tool for studying interstellar turbulence
• The resolved stellar populations in the LEGUS galaxies
• Spiral shocks, triggering of star formation and the velocity dispersion in Giant Molecular Clouds
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• The Role of Magnetic Fields in Protostellar Outflows and Star Formation
• Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scale
• Stellar feedback efficiencies: supernovae versus stellar winds
• Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
• Probing the evolution of molecular cloud structure II: From chaos to confinement
• A supersonic turbulence origin of Larson's laws
• Evolution of Magnetic Fields in High Mass Star Formation: Linking field geometry and collapse for the W51 e2/e8 cores
• Simulations of the Milky Way's central molecular zone -- II. Star formation
• Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds
• Incorporating the molecular gas phase in galaxy-size numerical simulations: first applications in dwarf galaxies
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics
• Supersonic turbulence, filamentary accretion,and the rapid assembly of massive stars and disks
• Mass inflow rate into the Central Molecular Zone: observational determination and evidence of episodic accretion
• Astrophysical turbulence modeling
• Millimeter-Wave Line Ratios and Sub-beam Volume Density Distributions
• Star-formation in NGC 4038/4039 from broad- and narrow band photometry: Cluster Destruction?
• Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation
• The dynamical evolution of molecular clouds near the Galactic Centre - II. Spatial structure and kinematics of simulated clouds
• Magnetization of cloud cores and envelopes and other observational consequences of reconnection diffusion
• The Age, Stellar Content and Star Formation Timescale of the B59 Dense Core
• Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds
• Control of Star Formation in Galaxies by Gravitational Instability
• IC 3418: Star Formation in a Turbulent Wake
• Fragmentation of Shocked Flows: Gravity, Turbulence and Cooling
• Approximations for modelling CO chemistry in GMCs: a comparison of approaches
• The CARMA-NRO Orion Survey
• The effect of dust cooling on low-metallicity star-forming clouds
• On the Origin of Asymmetries in Bilateral Supernova Remnants
• ATLASGAL-selected massive clumps in the inner Galaxy: V. Temperature structure and evolution
• Large Area Mapping at 850 Microns. IV. Analysis of the Clump Distribution in the Orion B South Molecular Cloud
• The evolution of large cavities and disc eccentricity in circumbinary discs
• Testing Larson's relationships in massive clumps
• Preserving chemical signatures of primordial star formation in the first low-mass stars
• Importance of the Initial Conditions for Star Formation - II. Fragmentation Induced Starvation and Accretion Shielding
• The origin of physical variations in the star formation law
• Clump Lifetimes and the Initial Mass Function
• Cloudlet capture by Transitional Disk and FU Orionis stars
• Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
• Fully compressive tides in galaxy mergers
• Filament formation in wind-cloud interactions. I. Spherical clouds in uniform magnetic fields
• The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• Change of Magnetic Field$-$Gas Alignment at Gravity-Driven Alfvénic Transition in Molecular Clouds: Implications for Dust Polarization Observations
• Opacity broadening and interpretation of suprathermal CO linewidths: Macroscopic Turbulence and Tangled Molecular Clouds
• Protostellar Outflows and Radiative Feedback from Massive Stars. II. Feedback, Star Formation Efficiency, and Outflow Broadening
• Identifying quiescent compact objects in massive Galactic single-lined spectroscopic binaries
• Gravitational Runaway and Turbulence Driving in Star-Gas Galactic Disks
• Evidence for a non-universal Kennicutt-Schmidt relationship using hierarchical Bayesian linear regression
• Physical Processes in Star Formation
• Spitzer mapping of molecular hydrogen pure rotational lines in NGC 1333: A detailed study of feedback in star formation
• Formation of quasi-periodic slow magnetoacoustic wave trains by the heating/cooling misbalance
• Star Formation Laws: the Effects of Gas Cloud Sampling
• Submillimeter Array Observations of Magnetic Fields in G240.31+0.07: an Hourglass in a Massive Cluster-forming Core
• On the self-regulation of intense star-formation in galaxies at z=1-3
• Cloud and Star Formation in Disk Galaxy Models with Feedback
• Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region
• Positron transport in the interstellar medium
• Magnetically Regulated Star Formation in Turbulent Clouds
• Saturation of the Turbulent Dynamo
• The Evolution and Properties of Rotating Massive Star Populations
• Collimated jets from the first core
• WARPFIELD 2.0: Feedback-regulated minimum star formation efficiencies of giant molecular clouds
• The formation and dynamical evolution of young star clusters
• How multiple supernovae overlap to form superbubbles
• The Nature of the Velocity Field in Molecular Clouds. I. The Non-Magnetic Case
• Turbulent Gas Flows in the Rosette and G216-2.5 Molecular Clouds: Assessing Turbulent Fragmentation Descriptions of Star Formation
• The structure and statistics of interstellar turbulence
• What controls the ionized gas turbulent motions in dwarf galaxies?
• Age spreads in star forming regions: The lithium test in the Orion Nebula Cluster
• The turbulent formation of stars
• Turbulence in the Interstellar Medium
• Magnetic Field Amplification in Young Galaxies
• Formation of the first stars and black holes
• Magnetohydrodynamic Simulations of Shock Interactions with Radiative Clouds
• The turbulent destruction of clouds - I. A k-epsilon treatment of turbulence in 2D models of adiabatic shock-cloud interactions
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• Dense core properties in the Infrared Dark cloud G14.225-0.506 revealed by ALMA
• Distribution of velocity gradient orientations: Mapping magnetization with the Velocity Gradient Technique
• The Complex Distribution of Recently Formed Stars. Bimodal Stellar Clustering in the Star-Forming Region NGC 346
• An Evolutionary Model for Collapsing Molecular Clouds and Their Star Formation Activity
• On the formation of density filaments in the turbulent interstellar medium
• Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media
• Damping of Alfven waves by Turbulence and its Consequences: from Cosmic-Rays Streaming to Launching Winds
• The role of molecular filaments in the origin of the prestellar core mass function and stellar initial mass function
• High resolution studies of massive primordial haloes
• Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
• Properties of Interstellar Turbulence from Gradients of Linear Radio Polarization Maps
• Supernova Feedback and the Hot Gas Filling Fraction of the Interstellar Medium
• A Fluid-Dynamical Subgrid Scale Model for Highly Compressible Astrophysical Turbulence
• Magneto-Hydrodynamics of Population III Star Formation
• Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements
• Star Formation in the First Galaxies - II: Clustered Star Formation and the Influence of Metal Line Cooling
• CARMA Large Area Star Formation Survey: Structure and Kinematics of Dense Gas in Serpens Main
• Age, size, and position of H ii regions in the Galaxy. Expansion of ionized gas in turbulent molecular clouds
• Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
• Magnetic Fields and Ionized Gas in the inner Galaxy: An Outer Scale for Turbulence and the Possible Role of HII Regions
• Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
• Pressure Support in Galaxy Disks: Impact on Rotation Curves and Dark Matter Density Profiles
• Review of Zeeman Effect Observations of Regions of Star Formation
• The SILCC project - V. The impact of magnetic fields on the chemistry and the formation of molecular clouds
• Magnetic Field Structure around Low-Mass Class 0 Protostars: B335, L1527 and IC348-SMM2
• The Minimum Mass for Opacity-Limited Fragmentation in Turbulent Cloud Cores
• Protostellar mass accretion rates from gravoturbulent fragmentation
• Evolution of Magnetic Fields in High Mass Star Formation: SMA dust polarization image of the UCHII region G5.89-0.39
• Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51
• Can Protostellar Jets Drive Supersonic Turbulence in Molecular Clouds?
• The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
• Which feedback mechanisms dominate in the high-pressure environment of the Central Molecular Zone?
• The morphology of the Milky Way - I. Reconstructing CO maps from simulations in fixed potentials
• The Free-Fall time of finite Sheets and Filaments
• Radial gas motions in The HI Nearby Galaxy Survey (THINGS)
• MHD Turbulence
• Molecular line mapping of the giant molecular cloud associated with RCW 106 - III. Multi-molecular line mapping
• Unbound Young Stellar Systems: Star Formation on the loose
• THOR - The HI, OH, Recombination Line Survey of the Milky Way - The pilot study: HI observations of the giant molecular cloud W43
• The Stellar Mass Spectrum in Warm and Dusty Gas: Deviations from Salpeter in the Galactic Centre and in Circum-Nuclear Starburst Regions
• On column density thresholds and the star formation rate
• Core-Halo Age Gradients and Star Formation in the Orion Nebula and NGC~2024 Young Stellar Clusters
• The Hall effect in star formation
• Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies
• Interstellar filaments and star formation
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: II. Comparison with Observation, Clump Properties, and Scaling to Physical Units
• On the effect of cosmological inflow on turbulence and instability in galactic discs
• Hierarchical fragmentation in the Perseus molecular cloud: From the cloud scale to protostellar objects
• Properties of dense cores in clustered massive star-forming regions at high angular resolution
• Generalized Collapse Solutions with Nonzero Initial Velocities for Star Formation in Molecular Cloud Cores
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• Kinematics of OB-associations in Gaia epoch
• Dark cloud cores and gravitational decoupling from turbulent flows
• HI velocity dispersion in NGC 1058
• Expanding molecular bubble surrounding Tycho's supernova remnant (SN 1572) observed with IRAM 30 m telescope: evidence for a single-degenerate progenitor
• M82, Starbursts, Star Clusters, and the Formation of Globular Clusters
• Star formation triggered by galaxy interactions in modified gravity
• Mapping Luminous Hot Stars in the Galaxy
• ALMA resolves the hourglass magnetic field in G31.41+0.31
• A 500 pc filamentary gas wisp in the disk of the Milky Way
• Studying Turbulence from Doppler-broadened Absorption Lines: Statistics of Logarithms of Intensity
• Embedded Star Clusters in the W51 Giant Molecular Cloud
• The pressure distribution in thermally bistable turbulent flows
• Fragmentation and Evolution of Molecular Clouds. I: Algorithm and First Results
• On the Structure of the Turbulent Interstellar Clouds
• The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds
• Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models
• Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks
• Larson's scaling laws, and the gravitational instability of clumpy discs at high redshift
• Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing
• On the Indeterministic Nature of Star Formation on the Cloud Scale
• Molecular Gas, Kinematics, and OB Star Formation in the Spiral Arms of the Southern Milky Way
• Local Simulations of Spiral Galaxies with the TIGRESS Framework: I. Star Formation and Arm Spurs/Feathers
• The Elongations and Supersonic Motions of Molecular Clouds
• On the formation of very metal-poor stars: The case of SDSS J1029151+172927
• Protostar Formation in Supersonic Flows: Growth and Collapse of Spherical Cores
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• Turbulence Spectra from Spectral Lines: Tests of the Velocity Channel Analysis and Velocity Coordinate Spectrum Techniques
• Turbulent Mixing in the Interstellar Medium -- an application for Lagrangian Tracer Particles
• The star formation efficiency and its relation to variations in the initial mass function
• Gas Properties and Implications for Galactic Star Formation in Numerical Models of the Turbulent, Multiphase ISM
• Observational consequences of turbulent pressure in the envelopes of massive stars
• Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields
• Amplification of Interstellar Magnetic Fields and Turbulent Mixing by Supernova-Driven Turbulence Part II - The Role of Dynamical Chaos
• Centrally Condensed Collapse of Starless Cores
• What sets the massive star formation rates and efficiencies of giant molecular clouds?
• Measuring the Alfvenic Nature of the Interstellar Medium: Velocity Anisotropy Revisited
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• Kinematic structure of massive star-forming regions - I. Accretion along filaments
• The Keele-Exeter young cluster survey: I. Low mass pre-main sequence stars in NGC 2169
• Kinematics of the Atomic ISM in M33 on 80 pc scales
• The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $\rho$ Ophiuchus C
• Scatter broadening of pulsars and implications on the interstellar medium turbulence
• SILCC-ZOOM: The early impact of ionizing radiation on forming molecular clouds
• The Gaia-ESO Survey and CSI 2264: Substructures, disks, and sequential star formation in the young open cluster NGC 2264
• Standard Self-Confinement and Extrinsic Turbulence Models for Cosmic Ray Transport are Fundamentally Incompatible with Observations
• Turbulent dynamo in the two-phase interstellar medium
• On the formation of trapezium-like systems
• Calibrating the Davis-Chandrasekhar-Fermi method with numerical simulations: uncertainties in estimating the magnetic field strength from statistics of field orientations
• Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds
• Magnetically-levitating disks around supermassive black holes
• Stellar Mass Spectra from Non-Isothermal Gravoturbulent Fragmentation
• Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
• Non-linear diffusion of cosmic rays escaping from supernova remnants - II. Hot ionized media
• Gradients of Synchrotron Polarization: Tracing 3D distribution of magnetic fields
• Can variability account for apparent age spreads in OB association colour-magnitude diagrams?
• The Nonisothermal Stage of Magnetic Star Formation. I. Formulation of the Problem and Method of Solution
• Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field
• Condition for the formation of micron-sized dust grains in dense molecular cloud cores
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• Protostellar Angular Momentum Evolution during Gravoturbulent Fragmentation
• Modelling of the Effects of Stellar Feedback during Star Cluster Formation Using a Hybrid Gas and N-Body Method
• A dynamical mechanism for the origin of nuclear rings
• Molecular clouds photoevaporation and FIR line emission
• Trans-Alfvenic Motions in the Taurus Molecular Cloud
• Properties of magnetohydrodynamic modes in compressively driven plasma turbulence
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• Gravity or turbulence? IV. Collapsing cores in out-of-virial disguise
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• The molecular complex associated with the Galactic HII region Sh2-90: a possible site of triggered star formation
• Physical properties and scaling relations of molecular clouds: the effect of stellar feedback
• Fragmentation in the First Galaxies
• Indications of a sub-linear and non-universal Kennicutt-Schmidt relationship
• Star Cluster Survival in Star Cluster Complexes under Extreme Residual Gas Expulsion
• Supersonic turbulence in shock-bound interaction zones I: symmetric settings
• Collisional N-Body Dynamics Coupled to Self-Gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation
• The fractal dimension of star-forming regions at different spatial scales in M33
• Supernova Feedback in Molecular Clouds: Global Evolution and Dynamics
• Velocity Anisotropy as a Diagnostic of the Magnetization of the Interstellar Medium and Molecular clouds
• The Effect of Star Formation History on the Inferred Initial Stellar Mass Function
• The supernova remnant population of the Small Magellanic Cloud
• Characterizing gravitational instability in turbulent multi-component galactic discs
• The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP
• Beyond the nuclear starburst? Clustered star formation in major mergers
• Simulating radiative feedback and star cluster formation in GMCs: I. Dependence on gravitational boundedness
• Herschel Observations of a Potential Core Forming Clump: Perseus B1-E
• Resolving Gas Dynamics in the Circumnuclear Region of a Disk Galaxy in a Cosmological Simulation
• Low energy cosmic rays
• Constraints on the formation mechanism of the planetary mass companion of 2MASS 1207334-393254
• Mapping the core mass function to the initial mass function
• The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies
• Interstellar Turbulence Driving by Galactic Spiral Shocks
• Dust-polarization maps for local interstellar turbulence
• Variable Accretion Rates and Fluffy First Stars
• The effect of magnetic fields on the formation of circumstellar discs around young stars
• Detections of CO in Late-Type, Low Surface Brightness Spiral Galaxies
• On the feedback from super stellar clusters. I. The structure of giant HII regions and HII galaxies
• The Small-Scale Dynamo at Low Magnetic Prandtl Numbers
• Forced turbulence in thermally bistable gas: A parameter study
• WISDOM Project -- X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
• Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
• Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• Millimeter interferometry of W3 IRS5: A Trapezium in the making
• Is molecular cloud turbulence driven by external supernova explosions?
• Seed magnetic fields in turbulent small-scale dynamos
• Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC18310-4
• Dynamo coefficients from local simulations of the turbulent ISM
• From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
• A Case Study of Low-Mass Star Formation
• High-resolution simulations of clump-clump collisions using SPH with Particle Splitting
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties
• Gaseous Spiral Structure and Mass Drift in Spiral Galaxies
• Spiral shocks and the formation of molecular clouds in a two phase medium
• Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code
• Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
• HI Power Spectra and the Turbulent ISM of Dwarf Irregular Galaxies
• Simulating field-aligned diffusion of a cosmic ray gas
• Shock Waves and Energy Dissipation in Magnetohydrodynamic Turbulence
• Formation of collapsing cores in subcritical magnetic clouds: three-dimensional MHD simulations with ambipolar diffusion
• Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium
• Cosmic-ray propagation in the bi-stable interstellar medium. I. Conditions for cosmic-ray trapping
• Plasma Diagnostics of the Interstellar Medium with Radio Astronomy
• WISDOM Project -- IX Giant Molecular Clouds in the Lenticular Galaxy NGC4429: Effects of Shear and Tidal Forces on Clouds
• 3D Continuum radiative transfer in complex dust configurations around young stellar objects and active nuclei II. 3D Structure of the dense molecular cloud core Rho Oph D
• Morphology and enhanced star formation in a Cartwheel-like ring galaxy
• WARPFIELD-EMP: The Self-Consistent Prediction of Emission Lines from Evolving HII Regions in Dense Molecular Clouds
• A quantification of the non-spherical geometry and accretion of collapsing cores
• The thinnest cold HI clouds in the diffuse interstellar medium?
• The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
• A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines
• Why Do Stars Form In Clusters? An Analytic Model for Stellar Correlation Functions
• Protostar Mass Due to Infall and Dispersal
• Wolf-Rayet and O Star Runaway Populations from Supernovae
• The Detection and Characterization of cm Radio Continuum Emission from the Low-mass Protostar L1014-IRS
• Hierarchical star formation across the grand design spiral NGC1566
• Parsec-scale structures and diffuse bands in a translucent interstellar medium at z 0.079
• When H II Regions are Complicated: Considering Perturbations from Winds, Radiation Pressure, and Other Effects
• Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas
• Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
• GASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud
• Density profile evolution during prestellar core collapse: Collapse starts at the large scale
• Testing kinematic distances under a realistic Galactic potential
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Molecular Tracers of Turbulent Shocks in Giant Molecular Clouds
• Hierarchical Stellar Structures in the Local Group Dwarf Galaxy NGC 6822
• The JCMT BISTRO Survey: The Distribution of Magnetic Field Strengths towards the OMC-1 Region
• Shock interactions, turbulence, and the origin of the stellar mass spectrum
• Magnetic field properties in star formation: a review of their analysis methods and interpretation
• Star Formation in Molecular Clouds
• The SAMI Galaxy Survey: Gas velocity dispersions in low-$z$ star-forming galaxies and the drivers of turbulence
• Constraining the Earliest Circumstellar Disks and their Envelopes
• The roles of stellar feedback and galactic environment in star forming molecular clouds
• The Clustering Behavior of Pre-Main Sequence Stars in NGC 346 in the Small Magellanic Cloud
• A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• Biases on initial mass function determinations. III. Cluster masses derived from unresolved photometry
• Study of velocity centroids based on the theory of fluctuations in position-position-velocity space
• ALMA ${}^{12}$CO (J=1--0) imaging of the nearby galaxy M83: Variations in the efficiency of star formation in giant molecular clouds
• Local Star formation triggered by SN shocks in magnetized diffuse neutral clouds
• The history of dynamics and stellar feedback revealed by the HI filamentary structure in the disk of the Milky Way
• Nonlinear Evolution of Gravitational Fragmentation Regulated by Magnetic Fields and Ambipolar Diffusion
• Close Stellar Encounters in Young, Substructured, Dissolving Star Clusters: Statistics and Effects on Planetary Systems
• Gaia Stellar Kinematics in the Head of the Orion A Cloud: Runaway Stellar Groups and Gravitational Infall
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• Protostellar collapse and fragmentation using an MHD GADGET
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• Jeans instability criterion modified by external tidal field
• Structure and Expansion Law of HII Regions in structured Molecular Clouds
• A physical approach to modelling large-scale galactic magnetic fields
• Simulations of cosmic ray propagation
• Protostellar Outflow Evolution in Turbulent Environments
• Star formation triggered by SN explosions: an application to the stellar association of $\beta$ Pictoris
• Magnetic field fluctuations in anisotropic, supersonic turbulence
• A SiO J = 5 - 4 Survey Toward Massive Star Formation Regions
• The Initial Conditions of Clustered Star Formation III. The Deuterium Fractionation of the Ophiuchus B2 Core
• 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 Survey of Centaurus A's Baryonic Structures (SCABS). II. The Extended Globular Cluster System of NGC5128 and its Nearby Environment
• Revealing Gravitational Collapse in Serpens G3-G6 Molecular Cloud using Velocity Gradients
• The 30 Doradus Molecular Cloud at 0.4 pc Resolution with the Atacama Large Millimeter/submillimeter Array: Physical Properties and the Boundedness of CO-emitting Structures
• Simulating Supersonic Turbulence in Galaxy Outflows
• Molecular Emission Line Formation in Prestellar Cores
• Non-ideal magnetohydrodynamics vs turbulence I: Which is the dominant process in protostellar disc formation?
• HII regions and high-mass starless clump candidates II. Fragmentation and induced star formation at ~0.025 pc scale: An ALMA continuum study
• Can WNM survive inside Molecular Clouds ?
• A revolution in star cluster research: setting the scene
• Simulations of momentum feedback by black hole winds
• Structure and kinematics of a massive galaxy at z ~ 7
• Statistics of Core Lifetimes in Numerical Simulations of Turbulent, Magnetically Supercritical Molecular Clouds
• Smoothed particle magnetohydrodynamic simulations of protostellar outflows with misaligned magnetic field and rotation axes
• Formation of the First Low-Mass Stars from Cosmological Initial Conditions
• Dissipative structures of diffuse molecular gas III -- Small-scale intermittency of intense velocity-shears
• Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
• Relations Between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud
• The Gaia-ESO Survey: age spread in the star forming region NGC6530 from the HR diagram and gravity indicators
• Giant Molecular Clouds in the Spiral Arm of IC 342
• Supersonic Cloud Collision - I
• The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation and magnetic walls during the early stages of star formation
• Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
• Clumpy and fractal shocks, and the generation of a velocity dispersion in molecular clouds
• Turbulent Magnetic Field Amplification by the Interaction of Shock Wave and Inhomogeneous Medium
• Mach number study of supersonic turbulence: The properties of the density field
• The Origin of Interstellar Turbulence in M33
• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• Shock generated vorticity in the interstellar medium and the origin of the stellar initial mass function
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Nobeyama 45-m mapping observations toward nearby molecular clouds, Orion A, Aquila Rift, and M17: Project overview
• Measuring Turbulence with Young Stars in the Orion Complex
• Catalogue of far-infrared loops in the Galaxy
• Gas expulsion in highly substructured embedded star clusters
• Variations in the ${\Sigma }_{\mathrm{SFR}}-{\Sigma }_{\mathrm{mol}}-{\Sigma }_{\star }$ plane across galactic environments in PHANGS galaxies
• Magnetic field structure around cores with very low luminosity objects
• The IMF as a function of supersonic turbulence
• Anisotropies in Compressible MHD Turbulence: Probing Magnetic Fields and Measuring Magnetization
• Thermal emission from bow shocks I: 2D Hydrodynamic Models of the Bubble Nebula
• Gravitational Instability in Radiation Pressure Dominated Backgrounds
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• On the origin of magnetic fields in stars
• Turbulence in Milky Way Star-Forming Regions Traced by Young Stars and Gas
• A large-scale CO survey of the Rosette Molecular Cloud: assessing the effects of O stars on surrounding molecular gas
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. I. The unmagnetized and zero-feedback limit
• Massive Star Forming Regions in the Galaxy using the Spitzer GLIMPSE Survey
• Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
• Shock-multicloud interactions in galactic outflows -- I. Cloud layers with log-normal density distributions
• Dynamical Expansion of H II Regions from Ultracompact to Compact Sizes in Turbulent, Self-Gravitating Molecular Clouds
• Formation of the first stars
• Damping of MHD turbulence in partially ionized gas and the observed difference of velocities of neutrals and ions
• The JCMT Gould Belt Survey: First results from SCUBA-2 observations of the Cepheus Flare Region
• A Catalog of HI Clouds in the Large Magellanic Cloud
• The Origin of Exponential Star-forming Disks
• The formation of protostellar binaries in primordial minihalos
• The Magnetic Field of Cloud 3 in L204
• The Turbulent Interstellar Medium
• Merging time-scales of stellar sub-clumps in young star-forming regions
• ALMA observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud
• MHD simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability
• Galactic synchrotron emission and the FIR-radio correlation at high redshift
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• On the turbulence driving mode of expanding HII regions
• The "Carina Flare" Supershell: Probing the Atomic and Molecular ISM in a Galactic Chimney
• Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC7 with Gaia EDR3: Evidence of Supernova Quenching
• Gravity and rotation drag the magnetic field in high-mass star formation
• Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds
• A multi-shock model for the density variance of anisotropic, highly-magnetised, supersonic turbulence
• Compressible turbulence in the interstellar medium: New insights from a high-resolution supersonic turbulence simulation
• Radiative transfer with POLARIS. II.: Modeling of synthetic Galactic synchrotron observations
• Curvature of magnetic field lines in compressible magnetized turbulence: Statistics, magnetization predictions, gradient curvature, modes and self-gravitating media
• Polarimetric studies of magnetic turbulence with interferometer
• Cosmic Ray propagation in sub-Alfvenic magnetohydrodynamic turbulence
• The Shapes of Molecular Cloud Cores in Orion
• Supernova-regulated ISM -- V. Space- and time-correlations
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• Flow-Driven Cloud Formation and Fragmentation: Results From Eulerian and Lagrangian Simulations
• Power Spectra in V-band and Halpha of Nine Irregular Galaxies
• Dynamical cloud formation traced by atomic and molecular gas
• Low-mass galaxy formation in cosmological AMR simulations: the effects of varying the sub-grid physics parameters
• On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions
• Young and intermediate-age massive star clusters
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: I. Formulation of the Problem and Method of Solution
• The clustered nature of star formation. Pre--main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud
• An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
• The Gas Properties of the W3 GMC: A HARP study
• Cloud formation in colliding flows: influence of the choice of cooling function
• Studying Magnetohydrodynamic Turbulence with Synchrotron Polarization Dispersion
• The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification
• Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
• Effects of dust absorption on spectroscopic studies of turbulence
• Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust
• Numerical simulations of supernova remnants in turbulent molecular clouds
• The Simons Observatory: Galactic Science Goals and Forecasts
• C18O Depletion in Starless Cores in Taurus
• Photoionisation and Heating of a Supernova Driven, Turbulent, Interstellar Medium
• Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• Statistical tracing of magnetic fields: comparing and improving the techniques
• The Gas-phase Metallicity Profiles of Star-forming Galaxies in the Modified Accretion Disk Framework
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• Density Power Spectrum in Turbulent Thermally Bi-stable Flows
• The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X
• Filament L1482 in the California molecular cloud
• The properties of Planck Galactic cold clumps in the L1495 dark cloud
• Infrared Radiation Feedback Does Not Regulate Star Cluster Formation
• Molecular cloud formation by compression of magnetized turbulent gas subjected to radiative cooling
• The driving of turbulence in simulations of molecular cloud formation and evolution
• Molecular cloud regulated star formation in galaxies
• Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling
• Direct Evidence for Two-Fluid Effects in Molecular Clouds
• Galactic magnetic fields and hierarchical galaxy formation
• Dichotomy in the Dynamical Status of Massive Cores in Orion
• Correlations Between Central Massive Objects And Their Host Galaxies: From Bulgeless Spirals to Ellipticals
• Kinematics and Structure of Star-forming Regions: Insights from Cold Collapse Models
• A semi-analytic model of the turbulent multi-phase interstellar medium
• Observational signatures of cosmic ray interactions in molecular clouds
• Evolution of Class0 protostars: Models vs. Observations
• Dependence of Hall Coefficient on Grain Size and Cosmic Ray Rate and Implication for Circumstellar Disk Formation
• Mapping molecular emission in Vela Molecular Ridge Cloud D
• Star formation efficiencies of molecular clouds in a galactic center environment
• Galactic Spiral Shocks with Thermal Instability in Vertically Stratified Galactic Disks
• The physical drivers of gas turbulence in simulated disc galaxies
• Gravity Versus Magnetic Fields in Forming Molecular Clouds
• Grammage of cosmic rays in the proximity of supernova remnants embedded in a partially ionized medium
• ALMA observations of RCW 120 Fragmentation at 0.01pc scale
• From large scale gas compression to cluster formation in the Antennae overlap region
• Connecting the Scales: Large Area High-resolution Ammonia Mapping of NGC 1333
• A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence
• The VMC Survey XXII. Hierarchical Star Formation in the 30 Doradus-N158-N159-N160 Star-Forming Complex
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
• A nonlinear structural subgrid-scale closure for compressible MHD Part II: a priori comparison on turbulence simulation data
• The small-scale dynamo in a multiphase supernova-driven medium
• Ambipolar Diffusion in Action: Transient C shock Structure and Prestellar Core Formation
• The Velocity Statistics of Turbulent Clouds in the Presence of Gravity, Magnetic fields, Radiation, and Outflow Feedback
• Dust continuum and Polarization from Envelope to Cores in Star Formation: A Case Study in the W51 North region
• The role of initial magnetic field structure in the launching of protostellar jets
• Criteria for gravitational instability and quasi-isolated gravitational collapse in turbulent medium
• Circumstellar Disks in the Outer Galaxy: the Star-Forming Region NGC 1893
• The Lyman alpha Reference Sample VI: Lyman alpha escape from the edge-on disk galaxy Mrk1486
• 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
• Simulations of the non-linear thin shell instability
• Tracing magnetic field morphology using the Velocity Gradient Technique in the presence of CO self-absorption
• Distortion of Magnetic Fields in a Starless Core: Near-Infrared Polarimetry of FeSt 1-457
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• Structure and Colors of Diffuse Emission in the Spitzer Galactic First Look Survey
• Modeling the kinematics of globular cluster systems
• Do we need non-ideal magnetohydrodynamics to model protostellar discs?
• Prestellar and protostellar cores in Ori B9
• LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
• Galactic fountains and outflows in star forming dwarf galaxies: ISM expulsion and chemical enrichment
• The onset of large scale turbulence in the interstellar medium of spiral galaxies
• Deuterium fractionation and H2D+ evolution in turbulent and magnetized cloud cores
• Accretion driven turbulence in filaments II: Effects of self-gravity
• Dimensional argument for the impact of turbulent support on the stellar initial mass function
• Measuring the filamentary structure of interstellar clouds through wavelets
• PHANGS: Constraining Star Formation Timescales Using the Spatial Correlations of Star Clusters and Giant Molecular Clouds
• Tracing Multi-Scale Magnetic Field Structure Using Multiple Chemical Tracers in Giant Molecular Clouds
• The Complex Large-scale Magnetic Fields in the First Galactic Quadrant as Revealed by the Faraday Depth Profile Disparity
• Sustaining star formation rates in spiral galaxies - Supernova-driven turbulent accretion disk models applied to THINGS galaxies
• Revealing HI gas in emission and absorption on pc to kpc scales in a galaxy at z ~ 0.017
• The Effect of Turbulence on Nebular Emission Line Ratios
• Stellar and substellar initial mass function: a model that implements gravoturbulent fragmentation and accretion
• Turbulence-induced magnetic fields in shock precursors
• Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
• Nonuniversal interstellar density spectra probed by pulsars
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• SOFIA observations of 30 Doradus: II -- Magnetic fields and large scale gas kinematics
• Mixing of Primordial Gas in Lyman Break Galaxies
• Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?
• Evidence for Dynamically Important Magnetic Fields in Molecular Clouds
• On the Origin of Multiple Populations During Massive Star Cluster Formation
• Alignment of the magnetic field in star forming regions and why it might be difficult to observe
• Hydrodynamical simulations of the decay of high-speed molecular turbulence. II. Divergence from isothermality
• Turbulence measurements from HI absorption spectra
• Interstellar MHD Turbulence and Star Formation
• Heightened Faraday Complexity in the inner 1 kpc of the Galactic Centre
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Driven Multifluid MHD Molecular Cloud Turbulence
• Synchrotron emission in molecular cloud cores: the SKA view
• A Radio Polarisation Study of Magnetic Fields in the Small Magellanic Cloud
• Non-adiabatic turbulence driving during gravitational collapse
• Magnetic tension and instabilities in the Orion A integral shaped filament
• Exact relations for energy transfer in self-gravitating isothermal turbulence
• The implications of dust for high-redshift protogalaxies and the formation of binary disks
• Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
• Multi-line observations of CH${}_3$OH, c-C${}_3$H${}_2$ and HNCO towards L1544: Dissecting the core structure with chemical differentiation
• Expanding CO Shells in the Orion A Molecular Cloud
• Kinematics of the molecular interstellar medium probed by Gaia: steep velocity dispersion-size relation, isotropic turbulence, and location-dependent energy dissipation
• Coreshine in L1506C - Evidence for a primitive big-grain component or indication for a turbulent core history?
• On the origin of magnetic fields in stars II: The effect of numerical resolution
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Early Evolution and 3D Structure of Embedded Star Clusters
• The organization of cloud-scale gas density structure: high resolution CO vs. 3.6 $\mu$m brightness contrasts in nearby galaxies
• Crescent-Shaped Molecular Outflow from the Intermediate-mass Protostar DK Cha Revealed by ALMA
• Incidence of HI 21-cm absorption in strong FeII systems at $0.5<z<1.5$
• Cluster Formation in Contracting Molecular Clouds
• The classical D-type expansion of spherical H II regions
• Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
• Jet-ISM Interactions near the Microquasars GRS 1758-258 and 1E 1740.7-2942
• Implementation of stellar heating feedback in simulations of star cluster formation: effects on the initial mass function
• A nonlinear structural subgrid-scale closure for compressible MHD Part I: derivation and energy dissipation properties
• Study Turbulence and Probe Magnetic Field Using Gradients Technique: Application to HI-to-H2 Transition Regions
• The Star Formation Law in a Multifractal ISM
• A submillimetre survey of the kinematics of the Perseus molecular cloud - III. Clump kinematics
• Star Formation in the Outer Galaxy: Coronal Properties of NGC 1893
• The relation between the true and observed fractal dimensions of turbulent clouds
• A Survey for Hydroxyl in the THOR Pilot Region around W43
• How do velocity structure functions trace gas dynamics in simulated molecular clouds?
• Signatures of fast and slow magnetohydrodynamic shocks in turbulent molecular clouds
• Velocity Gradients: Magnetic Field Tomography towards the Supernova Remnant W44
• Discovery of multi-seeded multi-mode formation of embedded clusters in the Rosette Molecular Complex
• Thermal structure of a protostellar envelope
• Ultra Violet Escape Fractions from Giant Molecular Clouds During Early Cluster Formation
• 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
• Evolution of circumstellar discs in young star-forming regions
• Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
• Spatial Power Spectra of Dust across the Local Group: No Constraint on Disc Scale Height
• Effects of turbulence and rotation on protostar formation as a precursor to seed black holes
• Dense Regions in Supersonic Isothermal Turbulence
• Dispersion of Observed Position Angles of Submillimeter Polarization in Molecular Clouds
• The small and the beautiful: How the star formation law affects galactic disk structure
• Physical properties of dense cores in Orion B9
• High-order semi-Lagrangian kinetic scheme for compressible turbulence
• The role of turbulence during the formation of circumbinary discs
• Centroid Velocity Statistics of Molecular Clouds
• PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction, $R_{\mathrm{mol}}$
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Understanding Galaxy Outflows as the Product of Unstable Turbulent Support
• On the maximum accretion rate of supermassive stars
• Fast deuterium fractionation in magnetized and turbulent filaments
• A comparison of shock-cloud and wind-cloud interactions: The longer survival of clouds in winds
• Mass-size scaling M~ r^1.67 of massive star-forming clumps -- evidences of turbulence-regulated gravitational collapse
• On the dissolution of star clusters in the Galactic centre. I. Circular orbits
• Searching for Molecular Outflows with Support Vector Machines: Dark Cloud Complex in Cygnus
• Generation of chiral asymmetry via helical magnetic fields
• Non-linear diffusion of cosmic rays escaping from supernova remnants: Cold partially neutral atomic and molecular phases
• The Catalogue for Astrophysical Turbulence Simulations (CATS)
• Revealing a spiral-shaped molecular cloud in our galaxy - Cloud fragmentation under rotation and gravity
• Insights from Simulations of Star Formation
• The magnetic field in the NGC 2024 FIR 5 dense core
• Atomic and molecular gas properties during cloud formation
• Mirror diffusion of cosmic rays in highly compressible turbulence near supernova remnants
• A molecular outflow evidencing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
• Nonlinear closures for scale separation in supersonic magnetohydrodynamic turbulence
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• Compression of turbulent magnetized gas in Giant Molecular Clouds
• Constructing multi-scale gravitational energy spectra from molecular cloud surface density PDF -- Interplay between turbulence and gravity
• Kinematics of Arp 270: gas flows, nuclear activity and two regimes of star formation
• Molecular cloud formation as seen in synthetic Hi and molecular gas observations
• Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action
• An Exploration of the Statistical Signatures of Stellar Feedback
• Galaxy Evolution: Modeling the Role of Non-thermal Pressure in the Interstellar medium
• Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE
• Dense Molecular Gas In A Young Cluster Around MWC 1080 -- Rule Of The Massive Star
• A Search for correlations between turbulence and star formation in LITTLE THINGS dwarf irregular galaxies
• The VMC Survey XXVII. Young Stellar Structures in the LMC${}^{\prime }$s Bar Star-Forming Complex
• The spectrum of magnetized turbulence in the interstellar medium
• Probing Three-Dimensional Magnetic Fields: I -- Polarized Dust Emission
• Studying the local magnetic field and anisotropy of magnetic turbulence by synchrotron polarization derivative
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• WISDOM Project -- XV. Giant Molecular Clouds in the Central Region of the Barred Spiral Galaxy NGC 5806
• Similarity between the C18O (J=1-0) core mass function and the IMF in the S 140 region
• Mapping the Galactic Magnetic Field Orientation and Strength in Three Dimensions
• CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
• The interaction of a magnetohydrodynamical shock with a filament
• The driving mode of shock-driven turbulence
• Morphological Dependence of Star Formation Properties for the Galaxies in the Merging Galaxy Cluster A2255
• Ionization front-driven turbulence in the clumpy interstellar medium
• Sheets, filaments and clumps - high resolution simulations of how the thermal instability can form molecular clouds
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
• Evidence of large scale energy cascade in the spiral galaxy NGC 5236
• Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
• Outflow - Core Interaction in Barnard 1
• Gas outflows in Seyfert galaxies: effects of star formation versus AGN feedbacks
• Spatial and dynamical structure of the NGC 2264 star-forming region
• Numerical viscosity and resistivity in MHD turbulence simulations
• A comparison of shock-cloud and wind-cloud interactions: effect of increased cloud density contrast on cloud evolution
• Probing the multi-scale interplay between gravity and turbulence - Power-law like gravitational energy spectra of the Orion Complex
• 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
• Magnetic fields in elliptical galaxies: Using the Laing-Garrington effect in radio galaxies and polarized emission from background radio sources
• Probing the magnetic fields in L1415 and L1389
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• The Interplay of Turbulence & Magnetic Fields in Star-Forming Regions: Simulations and Observations
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
• Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift
• Multi-Phase Magnetic Fields in the Galaxy NGC 3627
• Mass-density relationship in molecular cloud clumps
• Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
• Molecular Cloud Evolution
• Membership analysis and 3D kinematics of the star-forming complex around Trumpler 37 using Gaia-DR3
• Planck Cold Clumps in the lambda Orionis Complex. III. A chemical probe of stellar feedback on cores in the lambda Orionis cloud
• A comparison between Faraday Tomography and Synchrotron Polarization Gradients
• Accretion driven turbulence in filaments I: Non-gravitational accretion
• Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
• The effect of diffuse background on the spatially-resolved Schmidt relation in nearby spiral galaxies
• Supergiants and their shells in young globular clusters
• Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies
• Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity
• The location, clustering, and propagation of massive star formation in giant molecular clouds
• Studying Anisotropy of Compressible Magnetohydrodynamic Turbulence by Synchrotron Polarization Intensity
• Wide binary stars formed in the turbulent interstellar medium
• Magnetic Field Structure of the HH 1-2 Region: Near-Infrared Polarimetry of Point-Like Sources
• Kinematic signatures of cluster formation from cool collapse in the Lagoon Nebula cluster NGC 6530
• Spectral characterisation of inertial particle clustering in turbulence
• Modeling HI distribution and kinematics in the edge-on dwarf irregular galaxy KK250
• Evolution and lifetime of transient clumps in the turbulent interstellar medium
• Numerical Simulations of a Shock-Filament Interaction
• Precessing Jet and Large Dust Grains in the V380 Ori NE Star-forming Region
• Turbulence in Zeeman Measurements from Molecular Clouds
• HII regions and high-mass starless clump candidates I: Catalogs and properties
• Interstellar anatomy of the TeV gamma-ray peak in the IC443 supernova remnant
• Turbulence and Accretion: a High-resolution Study of the B5 Filaments
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• Multifluid magnetohydrodynamic turbulent decay
• Magnetic fields in star-forming systems (II): examining dust polarization, the Zeeman effect, and the Faraday rotation measure as magnetic field tracers
• A Survey of Magnetic Field Strengths in the Envelopes of Molecular Clouds via the 18 cm OH Zeeman Effect
• Role of Electon Excitation and Nature of Molecular Gas in Cluster Central Elliptical Galaxies
• Dynamical cooling of galactic discs by molecular cloud collisions -- Origin of giant clumps in gas-rich galaxy discs
• Kinetic and internal energy transfer in implicit large eddy simulations of forced compressible turbulence
• Toward Understanding the Origin of Turbulence in Molecular Clouds: Small Scale Structures as Units of Dynamical Multi-Phase Interstellar Medium
• Cloud Dispersal in Turbulent Flows
• Star formation in Chamaeleon I and III: a molecular line study of the starless core population
• Turbulence decay and cloud core relaxation in molecular clouds
• The Nature of Turbulence in the LITTLE THINGS Dwarf Irregular Galaxies
• Dynamo effect in unstirred self-gravitating turbulence
• Universal gravity-driven isothermal turbulence cascade in disk galaxies
• The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS)
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy
• Large-scale turbulent driving regulates star formation in high-redshift gas-rich galaxies II: Influence of the magnetic field and the turbulent compressive fraction
• A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
• Evolution of the angular momentum during gravitational fragmentation of molecular clouds
• Description of turbulent dynamics in the interstellar medium: multifractal/microcanonical analysis I. Application to Herschel observations of the Musca filament
• Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC7674
• Modelling the structure of molecular clouds: I. A multi-scale energy equipartition
• The JCMT Gould Belt Survey: Understanding the influence of molecular outflows on Gould Belt clouds
• Infall, outflow, and turbulence in massive star-forming cores in the G333 giant molecular cloud
• MRI-driven angular momentum transport in protoplanetary disks
• The Column Density Variance in Turbulent Interstellar Media: A Fractal Model Approach
• Filamentary Star Formation: Observing the Evolution toward Flattened Envelopes
• Clump mass function at an early stage of molecular cloud evolution: I. A statistical approach
• Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification
• Observations of chemical differentiation in clumpy molecular clouds
• Magnetic Field Strengths in Photodissociation Regions
• Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence
• Non-ideal MHD turbulent decay in molecular clouds
• Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence
• Dependence of the Star Formation Efficiency on the Parameters of Molecular Cloud Formation Simulations
• 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
• Quiescent Isolation: The Extremely Extended HI Halo of the Optically Compact Dwarf Galaxy ADBS 113845+2008
• A Search for correlations between turbulence and star formation in THINGS galaxies
• Probing Turbulence with Infrared Observations in OMC1
• TIMES I: a Systematic Observation in Multiple Molecular Lines Toward the Orion A and Ophiuchus Clouds
• Implementing and comparing sink particles in AMR and SPH
• Gravitational Fragmentation of Extremely Metal-poor Circumstellar Discs
• Intermittency of Fast MHD Modes and Regions of Anomalous Gradient Orientation in Low-beta Plasmas
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium
• The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 star-forming Clump
• High-resolution HI and CO observations of high-latitude intermediate-velocity clouds
• Necessary conditions for the formation of filaments and star clusters in the cold neutral medium
• Structure analysis of simulated molecular clouds with the Delta-variance
• Type III Societies (Apparently) Do Not Exist
• Radiation feedback in dusty clouds
• A Dynamically Collapsing Core and a Precursor of a Core in a Filament Supported by Turbulent and Magnetic Pressures
• Characterization of Turbulence from Submillimeter Dust Emission
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Starbursts and High-Redshift Galaxies are Radioactive: High Abundances of ${}^{26}$Al and Other Short Lived Radionuclides
• Distortion of Magnetic Fields in a Starless Core VI: Application of Flux Freezing Model and Core Formation of FeSt 1-457
• Generation of Solenoidal Modes and Magnetic Fields in Turbulence Driven by Compressive Driving
• On filament fragmentation and the impact of ambient environment on it
• The magnetic field in the dense photodissociation region of DR 21
• Spectroscopic Confirmation of a Population of Isolated, Intermediate-Mass YSOs
• Magnetic Flux Transport by turbulent reconnection in astrophysical flows
• Simulated observations of star formation regions: infrared evolution of globally collapsing clouds
• Gravity or turbulence V: Star forming regions undergoing violent relaxation
• Cloud properties across spatial scales in simulations of the interstellar medium
• Census of Gaseous Satellites around Local Spiral Galaxies
• Observational studies of pre-stellar cores and infrared dark clouds
• Inefficient star formation in high Mach number environments I. The turbulent support analytical model
• Number ratios of young stellar objects in embedded clusters
• Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds
• Interstellar Turbulence and Star Formation
• Numerical Simulations of a Protostellar Outflow Colliding with a Dense Molecular Cloud
• Formation of metal-free binaries: Impact of H${}_2$ line cooling and CIE cooling
• CO-0.30-0.07: A Peculiar Molecular Clump with an Extremely Broad Velocity Width
• Assessing the Impact of Astrochemistry on Molecular Cloud Turbulence Statistics
• Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
• Galactic Magnetic Turbulence from Radio data
• A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its variation on redshift and stellar mass
• The evolution of the internal structure of massive star forming regions in the Milky Way as revealed by ALMA
• Linear dust polarization during the embedded phase of protostar formation
• Bipolar molecular outflow of the very low-mass star Par-Lup3-4
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• The Interstellar Medium and Star Formation in Local Galaxies: Variations of the Star Formation Law in Simulations
• Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde V. The massive filament DR21
• The kinetic and magnetic energy budget of hub-filament systems during the gravitational fragmentation of molecular clouds
• The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
• Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei
• Centrally concentrated molecular gas driving galactic-scale ionised gas outflows in star-forming galaxies
• Testing assumptions and predictions of star-formation theories
• Interactions of a shock with a molecular cloud at various stages of its evolution due to thermal instability and gravity
• Simulations of pre-supernova feedback in spherical clouds
• Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
• Low-Mass Star Forming Cores in the GF9 Filament
• Density and Velocity Correlations in Isothermal Supersonic Turbulence
• Compact dusty clouds and efficient H${}_2$ formation in diffuse ISM
• DIISC-II: Unveiling the Connections between Star Formation and ISM in the Extended Ultraviolet Disk of NGC 3344
• Photoionization feedback in turbulent molecular clouds
• An ALMA search for substructure and fragmentation in starless cores in Orion B North
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• The influence of the cloud virial parameter on the initial mass function
• Chaotic behavior of Eulerian MHD turbulence
• Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS
• Characterizing star formation activity in infrared dark cloud MSXDC G048.65-00.29
• From Gas to Stars Over Cosmic Time
• Effects of the magnetic field direction on the Tsallis statistic
• The Astrochemical Evolution of Turbulent Giant Molecular Clouds : I - Physical Processes and Method of Solution for Hydrodynamic, Embedded Starless Clouds
• Exhaustion of the gas next to M31's supermassive black hole
• On the Functional Form of the Universal Star Formation Law
• Synthetic Observations of Carbon Lines of Turbulent Flows in Diffuse Multiphase Interstellar Medium
• Nonlinear Criterion for the Stability of Molecular Clouds
• Shocked Molecular Hydrogen and Broad CO lines from the Interacting Supernova Remnant HB 3
• The Spatial Power Spectrum and Derived Turbulent Properties of Isolated Galaxies
• Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
• CN Zeeman observations of the NGC 2264-C protocluster
• Can the removal of molecular cloud envelopes by external feedback affect the efficiency of star formation?
• OH maser toward IRAS 06056+2131: polarization parameters and evolution status
• Gradient measurement of synchrotron polarization diagnostic: Application to spatially separated emission and Faraday rotation regions
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• Statistical properties and correlation length in star-forming molecular clouds: I. Formalism and application to observations
• A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
• High resolution ALMA observation of the ${}^{12}$CO(3-2) and 350 GHz continuum emissions of the debris disc of 49 Ceti
• Angular Momentum Transport in Extended Galactic Disks
• Hubble-Lemaître fragmentation and the path to equilibrium of merger-driven cluster formation
• Formation of the First Galaxies: Theory and Simulations
• Open questions in the study of population III star formation
• Explosion Energies for Core-collapse Supernovae I: Analytic, Spherically Symmetric Solutions
• ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump
• The Degeneracy of Galaxy Formation Models
• IRAS 09002-4732: A Laboratory for the Formation of Rich Stellar Clusters
• Evolution of gaseous disk viscosity driven by supernova explosion. II. Structure and emissions from star-forming galaxies at high redshift
• Characterization of a turbulent flow with independent variation of Mach and Reynolds numbers
• Simultaneously modelling far-infrared dust emission and its relation to CO emission in star forming galaxies
• Star Formation at the Galactic Center
• Molecular Line Profiles from a Core Forming in a Turbulent Cloud
• Turbulence and its connection to episodic accretion in binary YSOs
• Multiwavelength Studies of Young OB Associations
• Mean fields and fluctuations in compressible magnetohydrodynamic flows
• Theories of the initial mass function
• Robustness of Synthetic Observations in Producing Observed Core Properties: Predictions for the TolTEC Clouds to Cores Legacy Survey
• Generalised transport equation of the Autocovariance Function of the density field and mass invariant in star-forming clouds
• Predicting HCN, HCO + , multi-transition CO, and dust emission of star-forming galaxies: Constraining the properties of resolved gas and dust disks of local spiral galaxies
• Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
• Inefficient star formation in high Mach number environments II. Numerical simulations and comparison with analytical models
• Scales of Stability and Turbulence in the Molecular ISM
• Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
• Deviation from a Continuous and Universal Turbulence Cascade in NGC 6334 due to Massive Star Formation Activity
• Differences in chemical evolution between isolated and embedded prestellar cores
• Density Exponent Analysis: Gravity-driven steepening of the density profiles of star-forming regions
• The High Rate of the Boyajian's Star Anomaly as a Phenomenon
• Initial Ionization of Compressible Turbulence
• Fragmentation and Structure Formation
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• A Deep Neural Network Approach to Compact Source Removal
• Dynamic duos: the building blocks of dimensional mechanics
• The magnetic field in the Flame nebula
• The turbulence driving parameter of molecular clouds in disc galaxies
• The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
• Star-forming environments in smoothed particle magnetohydrodynamics simulations I: Clump extraction and properties
• Turbulence driven by stellar jets, the possibility and the efficiency
• Formation of low-mass stars and brown dwarfs
• Massive star cluster formation III. Early mass segregation during cluster assembly
• Rubin LSST observing strategies to maximize volume and uniformity coverage of Star Forming Regions in the Galactic Plane
• 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
• Powerful flare phenomena in water vapor maser lines in the emerging protostellar system with protoplanetary disks IRAS 16293-2422
• Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
• Reconstructing the genesis of a globular cluster system at a look-back time of 9.1 Gyr with the JWST
• Studying Interstellar Turbulence Driving Scales using the Bispectrum
• Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences
• Relative Alignment Between Magnetic Fields and Molecular Gas Structure in Molecular Clouds
• Finite shock model of density in supersonic turbulence
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Line emission from filaments in molecular clouds
• Spiral arm triggering of star formation
• Impact of radiation feedback on the assembly of star clusters in galactic context
• Dust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains
• Studies of Dense Cores with ALMA
• Inverse Hubble Flows in Molecular Clouds
• Power spectra of outflow-driven turbulence
• The formation, disruption and properties of pressure-supported stellar systems and implications for the astrophysics of galaxies
• Simulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs
• Studying the properties of compressible MHD turbulence by synchrotron fluctuation statistics
• Density profile of a self-gravitating polytropic turbulent fluid in a rotating disk near to the cloud core
• Molecular Clouds Associated with {H \small{II}} regions and Candidates within l = 106.65${}^{\circ }$ to 109.50${}^{\circ }$ and b = $-$1.85${}^{\circ }$ to 0.95${}^{\circ }$
• Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
• 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
• Rydberg States of H${}_3$ and HeH as Potential Coolants for Primordial Star Formation
• Late encounter-events as a source of disks and spiral structures -- Forming second generation disks
• Understanding the IMF
• The Turbulent Interstellar Medium: Insights and Questions from Numerical Models
• Modeling the Disk (three-phase) Interstellar Medium
• Obtaining strength of magnetic field from E and B modes of dust polarization
• Measurement of the scaling slope of compressible magnetohydrodynamic turbulence by synchrotron radiation statistics
• Can galactic magnetic fields diffuse into the voids?
• Structure of iso-density sets in supersonic isothermal turbulence
• Turbulence in the Star-forming Interstellar Medium: Steps toward Constraining Theories with Observations
• A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity
• Magnetic fields and hot gas in M101
• Examining Turbulence in Galactic Molecular Clouds -- I: A Statistical Analysis of Velocity Structures
• Turbulent Control of the Star Formation Efficiency
• Statistical signatures of interstellar turbulence in dust polarization maps
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• Measuring the spectral index of turbulent gas with deep learning from projected density maps
• Anisotropy of Magnetohydrodynamic Turbulence and Polarization of the Spectral Lines of Molecules
• On the role of stochastic Fermi acceleration in setting the dissipation scale of turbulence in the interstellar medium
• The kinematics of the magnetised protostellar core IRAS15398-3359
• Molecular Fluctuations Inhibit Intermittency in Compressible Turbulence
• Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
• A Search for 3-mm Molecular Absorption Line Transitions in the Magellanic Stream
• Deuterium fractionation of the starless core L 1498
• From Gas to Stars over Cosmic Time
• Simulations of the IMF in Clusters
• A photo-ionized canopy for the shock-excited Criss-Cross Nebula
• Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations
• Magnetic Fields Studies in the Next Decade: EAO Submillimetre Futures White Paper Series, 2019
• Formation of star-forming clouds from the magnetised, diffuse interstellar medium
• Cloud fragmentation cascades and feedback: on reconciling an unfettered inertial range with a low star formation rate
• Young massive star clusters: Achievements and challenges
• Prospects of Turbulence Studies in High-Energy Density Laser-Generated Plasma: Numerical Investigations in Two Dimensions
• Molecular Cloud Turbulence And The Star Formation Efficiency: Enlarging the Scope
• Hydrodynamic and Magnetohydrodynamic Simulations of Wire Turbulence
• Primordial Black Holes Formed during Magneto-Hydrodynamic Turbulence in The Early Universe as Dominant Part of Dark Matter
• Stable smoothed particle magnetohydrodynamics in very steep density gradients
• Numerical Methods for Simulating Star Formation
• Observations of Protostellar Outflow Feedback in Clustered Star Formation
• A method for detection of structure
• Sound-Triggered Collapse of Stably Oscillating Low-Mass Cores in a Two-Phase Interstellar Medium
• Chemical chronology of the Southern Coalsack
• Bridging Theory and Observation: Synthetic Far-infrared Insights into Star Formation Efficiency
• Thermal damping of Weak Magnetosonic Turbulence in the Interstellar Medium
• Parallel and Perpendicular Alignments of Velocity Gradient and Magnetic Field observed in the Molecular Clouds L1478 and L1482
• The interdependence between density PDF, CMF and IMF and their relation with Mach number in simulations
• Vortex Detection from Quantum Data
• Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes
• Shock fragmentation model for gravitational collapse
• Heavy interstellar scattering toward the near end of the Galactic bar
• Mass Segregation in the CMZoom Survey
• From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data
• CO Structures with Narrow Lines in Nearby Quiescent Regions
• Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
• NH3 (1,1) hyperfine intensity anomalies in infall sources
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
• Magnetic fields in star forming environments: how does field strength affect gas on spiral arm and cloud scales?
• On the scale-height of the molecular gas disc in Milky Way-like galaxies
• Environmental Effects on the Dynamical Evolution of Star Clusters in Turbulent Molecular Clouds
• Self-confinement of low-energy cosmic rays around supernova remnants
• Supernova origin of galactic turbulence revealed by superbubbles
• Supernovae and photoionizing feedback in spiral arm molecular clouds
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies
• Why most molecular clouds are gravitationally dominated
• Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
• The signature of large scale turbulence driving on the structure of the interstellar medium
• A resolution criterion based on characteristic timescales for MHD simulations of molecular clouds
• Network of Star Formation: Fragmentation controlled by scale-dependent turbulent pressure and accretion onto the massive cores revealed in the Cygnus-X GMC complex
• Density profile of a self-gravitating polytropic turbulent fluid in the context of ensembles of molecular clouds
• Collapsing Index: A New Method to Identify Star-forming Cores Based on ALMA Images
• Thermal instability through the outer half of quasi-static spherically symmetric molecular clumps and cores
• On the interaction of a thin, supersonic shell with a molecular cloud
• A localized dynamic closure model for Euler turbulence
• Power spectrum to probe turbulence in Interstellar medium using 21cm line
• Cluster Density and the IMF
• The Numerical Simulation of Turbulence
• Cosmic Ray Propagation in Turbulent Spiral Magnetic Fields associated with Young Stellar Objects
• The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics
• On the structure of giant HII regions and HII galaxies
• Dynamical Evolution of a Supernova Driven Turbulent Interstellar Medium
• Turbulence in the Molecular Interstellar Medium
• On the star formation rate and turbulent dissipation in galactic models
• (Sub)mm Interferometry Applications in Star Formation Research
• Time Variability in Simulated Ultracompact and Hypercompact HII Regions
• The Supernova-ISM/Star formation Interplay
• Intermittency and non-universality of pair dispersion in isothermal compressible turbulence