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

References in corpus (17)

• The Formation Mechanism of Brown Dwarfs
• The Physics of Star Formation
• Star Formation from Galaxies to Globules
• The Formation of Close Binary Systems by Dynamical Interactions and Orbital Decay
• Flows, Fragmentation, and Star Formation. I. Low-mass Stars in Taurus
• Mixing Time Scales in a Supernova-Driven Interstellar Medium
• 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
• A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
• Gravity-driven Turbulence in Galactic Disks
• Dynamic cores in hydrostatic disguise
• 3D MHD Modeling of the Gaseous Structure of the Galaxy: Setup and Initial Results
• Structure Function Scaling of a 2MASS Extinction Map of Taurus
• Diffusion in supersonic, turbulent, compressible flows
• Constraints on star formation theories from the Serpens molecular cloud and protocluster
• Shapes of Molecular Cloud Cores and the Filamentary Mode of Star Formation
• Active star formation in N11B Nebula in the Large Magellanic Cloud: a sequential star formation scenario confirmed

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• Radial gas motions in The HI Nearby Galaxy Survey (THINGS)
• The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
• MHD Turbulence
• The Stellar Mass Spectrum in Warm and Dusty Gas: Deviations from Salpeter in the Galactic Centre and in Circum-Nuclear Starburst Regions
• Unbound Young Stellar Systems: Star Formation on the loose
• The Hall effect in star formation
• Core-Halo Age Gradients and Star Formation in the Orion Nebula and NGC~2024 Young Stellar Clusters
• THOR - The HI, OH, Recombination Line Survey of the Milky Way - The pilot study: HI observations of the giant molecular cloud W43
• On column density thresholds and the star formation rate
• Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies
• Interstellar filaments and star formation
• On the effect of cosmological inflow on turbulence and instability in galactic discs
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: II. Comparison with Observation, Clump Properties, and Scaling to Physical Units
• Generalized Collapse Solutions with Nonzero Initial Velocities for Star Formation in Molecular Cloud Cores
• Properties of dense cores in clustered massive star-forming regions at high angular resolution
• Hierarchical fragmentation in the Perseus molecular cloud: From the cloud scale to protostellar objects
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• Kinematics of OB-associations in Gaia epoch
• M82, Starbursts, Star Clusters, and the Formation of Globular Clusters
• Studying Turbulence from Doppler-broadened Absorption Lines: Statistics of Logarithms of Intensity
• A 500 pc filamentary gas wisp in the disk of the Milky Way
• Expanding molecular bubble surrounding Tycho's supernova remnant (SN 1572) observed with IRAM 30 m telescope: evidence for a single-degenerate progenitor
• Mapping Luminous Hot Stars in the Galaxy
• ALMA resolves the hourglass magnetic field in G31.41+0.31
• Star formation triggered by galaxy interactions in modified gravity
• Dark cloud cores and gravitational decoupling from turbulent flows
• HI velocity dispersion in NGC 1058
• The pressure distribution in thermally bistable turbulent flows
• On the Structure of the Turbulent Interstellar Clouds
• Fragmentation and Evolution of Molecular Clouds. I: Algorithm and First Results
• The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds
• Embedded Star Clusters in the W51 Giant Molecular Cloud
• Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks
• Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing
• Larson's scaling laws, and the gravitational instability of clumpy discs at high redshift
• Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models
• 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 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
• 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
• What sets the massive star formation rates and efficiencies of giant molecular clouds?
• Gas Properties and Implications for Galactic Star Formation in Numerical Models of the Turbulent, Multiphase ISM
• Turbulent Mixing in the Interstellar Medium -- an application for Lagrangian Tracer Particles
• Amplification of Interstellar Magnetic Fields and Turbulent Mixing by Supernova-Driven Turbulence Part II - The Role of Dynamical Chaos
• Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• Turbulence Spectra from Spectral Lines: Tests of the Velocity Channel Analysis and Velocity Coordinate Spectrum Techniques
• Centrally Condensed Collapse of Starless Cores
• 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
• Observational consequences of turbulent pressure in the envelopes of massive stars
• The star formation efficiency and its relation to variations in the initial mass function
• SILCC-ZOOM: The early impact of ionizing radiation on forming molecular clouds
• The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $\rho$ Ophiuchus C
• Kinematics of the Atomic ISM in M33 on 80 pc scales
• The Keele-Exeter young cluster survey: I. Low mass pre-main sequence stars in NGC 2169
• Scatter broadening of pulsars and implications on the interstellar medium turbulence
• Kinematic structure of massive star-forming regions - I. Accretion along filaments
• Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds
• Calibrating the Davis-Chandrasekhar-Fermi method with numerical simulations: uncertainties in estimating the magnetic field strength from statistics of field orientations
• Turbulent dynamo in the two-phase interstellar medium
• Standard Self-Confinement and Extrinsic Turbulence Models for Cosmic Ray Transport are Fundamentally Incompatible with Observations
• On the formation of trapezium-like systems
• The Gaia-ESO Survey and CSI 2264: Substructures, disks, and sequential star formation in the young open cluster NGC 2264
• Magnetically-levitating disks around supermassive black holes
• Formation of HI Clouds in Shock-compressed Interstellar Medium: Physical Origin of Angular Correlation Between Filamentary Structure and Magnetic Field
• Gradients of Synchrotron Polarization: Tracing 3D distribution of magnetic fields
• Stellar Mass Spectra from Non-Isothermal Gravoturbulent Fragmentation
• Non-linear diffusion of cosmic rays escaping from supernova remnants - II. Hot ionized media
• Can variability account for apparent age spreads in OB association colour-magnitude diagrams?
• Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
• Protostellar Angular Momentum Evolution during Gravoturbulent Fragmentation
• 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
• The Nonisothermal Stage of Magnetic Star Formation. I. Formulation of the Problem and Method of Solution
• Modelling of the Effects of Stellar Feedback during Star Cluster Formation Using a Hybrid Gas and N-Body Method
• Trans-Alfvenic Motions in the Taurus Molecular Cloud
• Properties of magnetohydrodynamic modes in compressively driven plasma turbulence
• A dynamical mechanism for the origin of nuclear rings
• Molecular clouds photoevaporation and FIR line emission
• Gravity or turbulence? IV. Collapsing cores in out-of-virial disguise
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• 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
• Supernova Feedback in Molecular Clouds: Global Evolution and Dynamics
• Star Cluster Survival in Star Cluster Complexes under Extreme Residual Gas Expulsion
• Fragmentation in the First Galaxies
• The Effect of Star Formation History on the Inferred Initial Stellar Mass Function
• Supersonic turbulence in shock-bound interaction zones I: symmetric settings
• Collisional N-Body Dynamics Coupled to Self-Gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation
• Indications of a sub-linear and non-universal Kennicutt-Schmidt relationship
• The fractal dimension of star-forming regions at different spatial scales in M33
• Velocity Anisotropy as a Diagnostic of the Magnetization of the Interstellar Medium and Molecular clouds
• The supernova remnant population of the Small Magellanic Cloud
• Characterizing gravitational instability in turbulent multi-component galactic discs
• Physical properties and scaling relations of molecular clouds: the effect of stellar feedback
• 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
• Low energy cosmic rays
• Resolving Gas Dynamics in the Circumnuclear Region of a Disk Galaxy in a Cosmological Simulation
• Beyond the nuclear starburst? Clustered star formation in major mergers
• The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP
• Dust-polarization maps for local interstellar turbulence
• On the feedback from super stellar clusters. I. The structure of giant HII regions and HII galaxies
• Forced turbulence in thermally bistable gas: A parameter study
• Interstellar Turbulence Driving by Galactic Spiral Shocks
• Variable Accretion Rates and Fluffy First Stars
• The Small-Scale Dynamo at Low Magnetic Prandtl Numbers
• Detections of CO in Late-Type, Low Surface Brightness Spiral Galaxies
• The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies
• Constraints on the formation mechanism of the planetary mass companion of 2MASS 1207334-393254
• The effect of magnetic fields on the formation of circumstellar discs around young stars
• Mapping the core mass function to the initial mass function
• WISDOM Project -- X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
• Millimeter interferometry of W3 IRS5: A Trapezium in the making
• Is molecular cloud turbulence driven by external supernova explosions?
• Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence
• A Case Study of Low-Mass Star Formation
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
• High-resolution simulations of clump-clump collisions using SPH with Particle Splitting
• Dynamo coefficients from local simulations of the turbulent ISM
• Seed magnetic fields in turbulent small-scale dynamos
• Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC18310-4
• Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties
• Simulating field-aligned diffusion of a cosmic ray gas
• HI Power Spectra and the Turbulent ISM of Dwarf Irregular Galaxies
• Gaseous Spiral Structure and Mass Drift in Spiral Galaxies
• Shock Waves and Energy Dissipation in Magnetohydrodynamic Turbulence
• Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
• 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
• 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
• 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
• WARPFIELD-EMP: The Self-Consistent Prediction of Emission Lines from Evolving HII Regions in Dense Molecular Clouds
• The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
• WISDOM Project -- IX Giant Molecular Clouds in the Lenticular Galaxy NGC4429: Effects of Shear and Tidal Forces on Clouds
• The thinnest cold HI clouds in the diffuse interstellar medium?
• A quantification of the non-spherical geometry and accretion of collapsing cores
• Morphology and enhanced star formation in a Cartwheel-like ring galaxy
• 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
• Wolf-Rayet and O Star Runaway Populations from Supernovae
• Parsec-scale structures and diffuse bands in a translucent interstellar medium at z 0.079
• 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
• Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas
• Density profile evolution during prestellar core collapse: Collapse starts at the large scale
• Hierarchical Stellar Structures in the Local Group Dwarf Galaxy NGC 6822
• When H II Regions are Complicated: Considering Perturbations from Winds, Radiation Pressure, and Other Effects
• GASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud
• Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
• Testing kinematic distances under a realistic Galactic potential
• Molecular Tracers of Turbulent Shocks in Giant Molecular Clouds
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Shock interactions, turbulence, and the origin of the stellar mass spectrum
• A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud
• Biases on initial mass function determinations. III. Cluster masses derived from unresolved photometry
• 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
• The roles of stellar feedback and galactic environment in star forming molecular clouds
• The JCMT BISTRO Survey: The Distribution of Magnetic Field Strengths towards the OMC-1 Region
• Constraining the Earliest Circumstellar Disks and their Envelopes
• Study of velocity centroids based on the theory of fluctuations in position-position-velocity space
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• The Clustering Behavior of Pre-Main Sequence Stars in NGC 346 in the Small Magellanic Cloud
• Nonlinear Evolution of Gravitational Fragmentation Regulated by Magnetic Fields and Ambipolar Diffusion
• Local Star formation triggered by SN shocks in magnetized diffuse neutral clouds
• 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
• The history of dynamics and stellar feedback revealed by the HI filamentary structure in the disk of the Milky Way
• ALMA ${}^{12}$CO (J=1--0) imaging of the nearby galaxy M83: Variations in the efficiency of star formation in giant molecular clouds
• Simulations of cosmic ray propagation
• Structure and Expansion Law of HII Regions in structured Molecular Clouds
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• A physical approach to modelling large-scale galactic magnetic fields
• Protostellar Outflow Evolution in Turbulent Environments
• Star formation triggered by SN explosions: an application to the stellar association of $\beta$ Pictoris
• Jeans instability criterion modified by external tidal field
• Protostellar collapse and fragmentation using an MHD GADGET
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• The Initial Conditions of Clustered Star Formation III. The Deuterium Fractionation of the Ophiuchus B2 Core
• Simulating Supersonic Turbulence in Galaxy Outflows
• Molecular Emission Line Formation in Prestellar Cores
• A SiO J = 5 - 4 Survey Toward Massive Star Formation Regions
• 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
• The Survey of Centaurus A's Baryonic Structures (SCABS). II. The Extended Globular Cluster System of NGC5128 and its Nearby Environment
• Magnetic field fluctuations in anisotropic, supersonic turbulence
• 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
• Revealing Gravitational Collapse in Serpens G3-G6 Molecular Cloud using Velocity Gradients
• 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
• HII regions and high-mass starless clump candidates II. Fragmentation and induced star formation at ~0.025 pc scale: An ALMA continuum study
• Non-ideal magnetohydrodynamics vs turbulence I: Which is the dominant process in protostellar disc formation?
• Can WNM survive inside Molecular Clouds ?
• Smoothed particle magnetohydrodynamic simulations of protostellar outflows with misaligned magnetic field and rotation axes
• A revolution in star cluster research: setting the scene
• Statistics of Core Lifetimes in Numerical Simulations of Turbulent, Magnetically Supercritical Molecular Clouds
• Simulations of momentum feedback by black hole winds
• Structure and kinematics of a massive galaxy at z ~ 7
• Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
• Giant Molecular Clouds in the Spiral Arm of IC 342
• The Gaia-ESO Survey: age spread in the star forming region NGC6530 from the HR diagram and gravity indicators
• The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation and magnetic walls during the early stages of star formation
• 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
• Clumpy and fractal shocks, and the generation of a velocity dispersion in molecular clouds
• Supersonic Cloud Collision - I
• Shock generated vorticity in the interstellar medium and the origin of the stellar initial mass function
• Catalogue of far-infrared loops in the Galaxy
• Mach number study of supersonic turbulence: The properties of the density field
• Measuring Turbulence with Young Stars in the Orion Complex
• The Origin of Interstellar Turbulence in M33
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Turbulent Magnetic Field Amplification by the Interaction of Shock Wave and Inhomogeneous Medium
• Nobeyama 45-m mapping observations toward nearby molecular clouds, Orion A, Aquila Rift, and M17: Project overview
• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• Gravitational Instability in Radiation Pressure Dominated Backgrounds
• Massive Star Forming Regions in the Galaxy using the Spitzer GLIMPSE Survey
• Thermal emission from bow shocks I: 2D Hydrodynamic Models of the Bubble Nebula
• The IMF as a function of supersonic turbulence
• A large-scale CO survey of the Rosette Molecular Cloud: assessing the effects of O stars on surrounding molecular gas
• Magnetic field structure around cores with very low luminosity objects
• Turbulence in Milky Way Star-Forming Regions Traced by Young Stars and Gas
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• Gas expulsion in highly substructured embedded star clusters
• Anisotropies in Compressible MHD Turbulence: Probing Magnetic Fields and Measuring Magnetization
• Variations in the ${\Sigma }_{\mathrm{SFR}}-{\Sigma }_{\mathrm{mol}}-{\Sigma }_{\star }$ plane across galactic environments in PHANGS galaxies
• On the origin of magnetic fields in stars
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. I. The unmagnetized and zero-feedback limit
• Formation of the first stars
• Massive star cluster formation I. High star formation efficiency while resolving feedback of individual 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
• Dynamical Expansion of H II Regions from Ultracompact to Compact Sizes in Turbulent, Self-Gravitating Molecular Clouds
• Shock-multicloud interactions in galactic outflows -- I. Cloud layers with log-normal density distributions
• MHD simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability
• Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC7 with Gaia EDR3: Evidence of Supernova Quenching
• Galactic synchrotron emission and the FIR-radio correlation at high redshift
• The Origin of Exponential Star-forming Disks
• A Catalog of HI Clouds in the Large Magellanic Cloud
• The formation of protostellar binaries in primordial minihalos
• The Turbulent Interstellar Medium
• On the turbulence driving mode of expanding HII regions
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• ALMA observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud
• Merging time-scales of stellar sub-clumps in young star-forming regions
• The Magnetic Field of Cloud 3 in L204
• The "Carina Flare" Supershell: Probing the Atomic and Molecular ISM in a Galactic Chimney
• Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds
• Radiative transfer with POLARIS. II.: Modeling of synthetic Galactic synchrotron observations
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Compressible turbulence in the interstellar medium: New insights from a high-resolution supersonic turbulence simulation
• Low-mass galaxy formation in cosmological AMR simulations: the effects of varying the sub-grid physics parameters
• Flow-Driven Cloud Formation and Fragmentation: Results From Eulerian and Lagrangian Simulations
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• Polarimetric studies of magnetic turbulence with interferometer
• Curvature of magnetic field lines in compressible magnetized turbulence: Statistics, magnetization predictions, gradient curvature, modes and self-gravitating media
• Cosmic Ray propagation in sub-Alfvenic magnetohydrodynamic turbulence
• On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions
• A multi-shock model for the density variance of anisotropic, highly-magnetised, supersonic turbulence
• Supernova-regulated ISM -- V. Space- and time-correlations
• The Shapes of Molecular Cloud Cores in Orion
• Gravity and rotation drag the magnetic field in high-mass star formation
• Power Spectra in V-band and Halpha of Nine Irregular Galaxies
• Dynamical cloud formation traced by atomic and molecular gas
• 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
• Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
• C18O Depletion in Starless Cores in Taurus
• An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
• Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust
• The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification
• The Simons Observatory: Galactic Science Goals and Forecasts
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: I. Formulation of the Problem and Method of Solution
• Young and intermediate-age massive star clusters
• Effects of dust absorption on spectroscopic studies of turbulence
• The clustered nature of star formation. Pre--main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud
• Numerical simulations of supernova remnants in turbulent molecular clouds
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• The Gas-phase Metallicity Profiles of Star-forming Galaxies in the Modified Accretion Disk Framework
• Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
• Photoionisation and Heating of a Supernova Driven, Turbulent, Interstellar Medium
• 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
• Molecular cloud regulated star formation in galaxies
• Direct Evidence for Two-Fluid Effects in Molecular Clouds
• 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
• Kinematics and Structure of Star-forming Regions: Insights from Cold Collapse Models
• Dichotomy in the Dynamical Status of Massive Cores in Orion
• Correlations Between Central Massive Objects And Their Host Galaxies: From Bulgeless Spirals to Ellipticals
• Filament L1482 in the California molecular cloud
• Infrared Radiation Feedback Does Not Regulate Star Cluster Formation
• Density Power Spectrum in Turbulent Thermally Bi-stable Flows
• Galactic magnetic fields and hierarchical galaxy formation
• The properties of Planck Galactic cold clumps in the L1495 dark cloud
• The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X
• Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling
• A semi-analytic model of the turbulent multi-phase interstellar medium
• A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence
• 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
• The physical drivers of gas turbulence in simulated disc galaxies
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• ALMA observations of RCW 120 Fragmentation at 0.01pc scale
• The VMC Survey XXII. Hierarchical Star Formation in the 30 Doradus-N158-N159-N160 Star-Forming Complex
• Observational signatures of cosmic ray interactions in molecular clouds
• Grammage of cosmic rays in the proximity of supernova remnants embedded in a partially ionized medium
• A nonlinear structural subgrid-scale closure for compressible MHD Part II: a priori comparison on turbulence simulation data
• Galactic Spiral Shocks with Thermal Instability in Vertically Stratified Galactic Disks
• The small-scale dynamo in a multiphase supernova-driven medium
• Gravity Versus Magnetic Fields in Forming Molecular Clouds
• Mapping molecular emission in Vela Molecular Ridge Cloud D
• SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
• Evolution of Class0 protostars: Models vs. Observations
• Star formation efficiencies of molecular clouds in a galactic center environment
• Dependence of Hall Coefficient on Grain Size and Cosmic Ray Rate and Implication for Circumstellar Disk Formation
• Ambipolar Diffusion in Action: Transient C shock Structure and Prestellar Core Formation
• Structure and Colors of Diffuse Emission in the Spitzer Galactic First Look Survey
• Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium
• Circumstellar Disks in the Outer Galaxy: the Star-Forming Region NGC 1893
• Dust continuum and Polarization from Envelope to Cores in Star Formation: A Case Study in the W51 North region
• Criteria for gravitational instability and quasi-isolated gravitational collapse in turbulent medium
• Distortion of Magnetic Fields in a Starless Core: Near-Infrared Polarimetry of FeSt 1-457
• Simulations of the non-linear thin shell instability
• The Lyman alpha Reference Sample VI: Lyman alpha escape from the edge-on disk galaxy Mrk1486
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• The role of initial magnetic field structure in the launching of protostellar jets
• Tracing magnetic field morphology using the Velocity Gradient Technique in the presence of CO self-absorption
• The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds
• The Velocity Statistics of Turbulent Clouds in the Presence of Gravity, Magnetic fields, Radiation, and Outflow Feedback
• Tracing Multi-Scale Magnetic Field Structure Using Multiple Chemical Tracers in Giant Molecular Clouds
• Galactic fountains and outflows in star forming dwarf galaxies: ISM expulsion and chemical enrichment
• Deuterium fractionation and H2D+ evolution in turbulent and magnetized cloud cores
• Do we need non-ideal magnetohydrodynamics to model protostellar discs?
• Prestellar and protostellar cores in Ori B9
• The onset of large scale turbulence in the interstellar medium of spiral galaxies
• LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
• Measuring the filamentary structure of interstellar clouds through wavelets
• Modeling the kinematics of globular cluster systems
• Accretion driven turbulence in filaments II: Effects of self-gravity
• PHANGS: Constraining Star Formation Timescales Using the Spatial Correlations of Star Clusters and Giant Molecular Clouds
• Dimensional argument for the impact of turbulent support on the stellar initial mass function
• The Effect of Turbulence on Nebular Emission Line Ratios
• Turbulence-induced magnetic fields in shock precursors
• Sustaining star formation rates in spiral galaxies - Supernova-driven turbulent accretion disk models applied to THINGS galaxies
• Nonuniversal interstellar density spectra probed by pulsars
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Stellar and substellar initial mass function: a model that implements gravoturbulent fragmentation and accretion
• The Complex Large-scale Magnetic Fields in the First Galactic Quadrant as Revealed by the Faraday Depth Profile Disparity
• Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• Revealing HI gas in emission and absorption on pc to kpc scales in a galaxy at z ~ 0.017
• Synchrotron emission in molecular cloud cores: the SKA view
• Alignment of the magnetic field in star forming regions and why it might be difficult to observe
• The implications of dust for high-redshift protogalaxies and the formation of binary disks
• Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?
• Heightened Faraday Complexity in the inner 1 kpc of the Galactic Centre
• Driven Multifluid MHD Molecular Cloud Turbulence
• Hydrodynamical simulations of the decay of high-speed molecular turbulence. II. Divergence from isothermality
• A Radio Polarisation Study of Magnetic Fields in the Small Magellanic Cloud
• Interstellar MHD Turbulence and Star Formation
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Exact relations for energy transfer in self-gravitating isothermal turbulence
• On the Origin of Multiple Populations During Massive Star Cluster Formation
• Evidence for Dynamically Important Magnetic Fields in Molecular Clouds
• Non-adiabatic turbulence driving during gravitational collapse
• Magnetic tension and instabilities in the Orion A integral shaped filament
• Mixing of Primordial Gas in Lyman Break Galaxies
• Less wrong: a more realistic initial condition for simulations of turbulent molecular clouds
• SOFIA observations of 30 Doradus: II -- Magnetic fields and large scale gas kinematics
• Turbulence measurements from HI absorption spectra
• The classical D-type expansion of spherical H II regions
• Incidence of HI 21-cm absorption in strong FeII systems at $0.5<z<1.5$
• Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
• The organization of cloud-scale gas density structure: high resolution CO vs. 3.6 $\mu$m brightness contrasts in nearby galaxies
• Multi-line observations of CH${}_3$OH, c-C${}_3$H${}_2$ and HNCO towards L1544: Dissecting the core structure with chemical differentiation
• On the origin of magnetic fields in stars II: The effect of numerical resolution
• Early Evolution and 3D Structure of Embedded Star Clusters
• 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
• Cluster Formation in Contracting Molecular Clouds
• Coreshine in L1506C - Evidence for a primitive big-grain component or indication for a turbulent core history?
• Crescent-Shaped Molecular Outflow from the Intermediate-mass Protostar DK Cha Revealed by ALMA
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• The Star Formation Law in a Multifractal ISM
• Signatures of fast and slow magnetohydrodynamic shocks in turbulent molecular clouds
• How do velocity structure functions trace gas dynamics in simulated molecular clouds?
• Study Turbulence and Probe Magnetic Field Using Gradients Technique: Application to HI-to-H2 Transition Regions
• 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
• Star Formation in the Outer Galaxy: Coronal Properties of NGC 1893
• A nonlinear structural subgrid-scale closure for compressible MHD Part I: derivation and energy dissipation properties
• A submillimetre survey of the kinematics of the Perseus molecular cloud - III. Clump kinematics
• A Survey for Hydroxyl in the THOR Pilot Region around W43
• The relation between the true and observed fractal dimensions of turbulent clouds
• 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
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• Simultaneous evolution of the virial parameter and star formation rate in molecular clumps undergoing global hierarchical collapse
• Ultra Violet Escape Fractions from Giant Molecular Clouds During Early Cluster Formation
• Evolution of circumstellar discs in young star-forming regions
• Velocity Gradients: Magnetic Field Tomography towards the Supernova Remnant W44
• 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
• The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
• Thermal structure of a protostellar envelope
• Dispersion of Observed Position Angles of Submillimeter Polarization in Molecular Clouds
• Dense Regions in Supersonic Isothermal Turbulence
• Discovery of multi-seeded multi-mode formation of embedded clusters in the Rosette Molecular Complex
• High-order semi-Lagrangian kinetic scheme for compressible turbulence
• On the maximum accretion rate of supermassive stars
• PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction, $R_{\mathrm{mol}}$
• The role of turbulence during the formation of circumbinary discs
• The small and the beautiful: How the star formation law affects galactic disk structure
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• Understanding Galaxy Outflows as the Product of Unstable Turbulent Support
• Centroid Velocity Statistics of Molecular Clouds
• Physical properties of dense cores in Orion B9
• Revealing a spiral-shaped molecular cloud in our galaxy - Cloud fragmentation under rotation and gravity
• Non-linear diffusion of cosmic rays escaping from supernova remnants: Cold partially neutral atomic and molecular phases
• The magnetic field in the NGC 2024 FIR 5 dense core
• Generation of chiral asymmetry via helical magnetic fields
• The Catalogue for Astrophysical Turbulence Simulations (CATS)
• Fast deuterium fractionation in magnetized and turbulent filaments
• A comparison of shock-cloud and wind-cloud interactions: The longer survival of clouds in winds
• Searching for Molecular Outflows with Support Vector Machines: Dark Cloud Complex in Cygnus
• Atomic and molecular gas properties during cloud formation
• Mirror diffusion of cosmic rays in highly compressible turbulence near supernova remnants
• Insights from Simulations of Star Formation
• Mass-size scaling M~ r^1.67 of massive star-forming clumps -- evidences of turbulence-regulated gravitational collapse
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• On the dissolution of star clusters in the Galactic centre. I. Circular orbits
• Nonlinear closures for scale separation in supersonic magnetohydrodynamic turbulence
• A molecular outflow evidencing star formation activity in the vicinity of the HII region G034.8-0.7 and the SNR W44
• Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action
• Compression of turbulent magnetized gas in Giant Molecular Clouds
• An Exploration of the Statistical Signatures of Stellar Feedback
• 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
• Constructing multi-scale gravitational energy spectra from molecular cloud surface density PDF -- Interplay between turbulence and gravity
• Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE
• Kinematics of Arp 270: gas flows, nuclear activity and two regimes of star formation
• Galaxy Evolution: Modeling the Role of Non-thermal Pressure in the Interstellar medium
• A Search for correlations between turbulence and star formation in LITTLE THINGS dwarf irregular galaxies
• Molecular cloud formation as seen in synthetic Hi and molecular gas observations
• Dense Molecular Gas In A Young Cluster Around MWC 1080 -- Rule Of The Massive Star
• The driving mode of shock-driven turbulence
• Probing Three-Dimensional Magnetic Fields: I -- Polarized Dust Emission
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• The interaction of a magnetohydrodynamical shock with a filament
• CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
• Similarity between the C18O (J=1-0) core mass function and the IMF in the S 140 region
• Ionization front-driven turbulence in the clumpy interstellar medium
• Studying the local magnetic field and anisotropy of magnetic turbulence by synchrotron polarization derivative
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• Mapping the Galactic Magnetic Field Orientation and Strength in Three Dimensions
• WISDOM Project -- XV. Giant Molecular Clouds in the Central Region of the Barred Spiral Galaxy NGC 5806
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• Sheets, filaments and clumps - high resolution simulations of how the thermal instability can form molecular clouds
• Morphological Dependence of Star Formation Properties for the Galaxies in the Merging Galaxy Cluster A2255
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• Gas outflows in Seyfert galaxies: effects of star formation versus AGN feedbacks
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement
• A new method for probing magnetic field strengths from striations in the interstellar medium
• Evidence of large scale energy cascade in the spiral galaxy NGC 5236
• Numerical viscosity and resistivity in MHD turbulence simulations
• Probing the multi-scale interplay between gravity and turbulence - Power-law like gravitational energy spectra of the Orion Complex
• Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift
• Outflow - Core Interaction in Barnard 1
• The Interplay of Turbulence & Magnetic Fields in Star-Forming Regions: Simulations and Observations
• Multi-Phase Magnetic Fields in the Galaxy NGC 3627
• WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
• Probing the magnetic fields in L1415 and L1389
• Magnetic fields in elliptical galaxies: Using the Laing-Garrington effect in radio galaxies and polarized emission from background radio sources
• A comparison of shock-cloud and wind-cloud interactions: effect of increased cloud density contrast on cloud evolution
• Mass-density relationship in molecular cloud clumps
• Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
• Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics?
• Spatial and dynamical structure of the NGC 2264 star-forming region
• Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
• Studying Anisotropy of Compressible Magnetohydrodynamic Turbulence by Synchrotron Polarization Intensity
• The effect of diffuse background on the spatially-resolved Schmidt relation in nearby spiral galaxies
• The location, clustering, and propagation of massive star formation in giant molecular clouds
• Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies
• Wide binary stars formed in the turbulent interstellar medium
• Membership analysis and 3D kinematics of the star-forming complex around Trumpler 37 using Gaia-DR3
• Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
• Spectral characterisation of inertial particle clustering in turbulence
• Planck Cold Clumps in the lambda Orionis Complex. III. A chemical probe of stellar feedback on cores in the lambda Orionis cloud
• Kinematic signatures of cluster formation from cool collapse in the Lagoon Nebula cluster NGC 6530
• A comparison between Faraday Tomography and Synchrotron Polarization Gradients
• Supergiants and their shells in young globular clusters
• Accretion driven turbulence in filaments I: Non-gravitational accretion
• Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity
• Modeling HI distribution and kinematics in the edge-on dwarf irregular galaxy KK250
• Molecular Cloud Evolution
• Evolution and lifetime of transient clumps in the turbulent interstellar medium
• Magnetic Field Structure of the HH 1-2 Region: Near-Infrared Polarimetry of Point-Like Sources
• Dynamical cooling of galactic discs by molecular cloud collisions -- Origin of giant clumps in gas-rich galaxy discs
• Numerical Simulations of a Shock-Filament Interaction
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• Precessing Jet and Large Dust Grains in the V380 Ori NE Star-forming Region
• Magnetic fields in star-forming systems (II): examining dust polarization, the Zeeman effect, and the Faraday rotation measure as magnetic field tracers
• Role of Electon Excitation and Nature of Molecular Gas in Cluster Central Elliptical Galaxies
• Turbulence in Zeeman Measurements from Molecular Clouds
• Interstellar anatomy of the TeV gamma-ray peak in the IC443 supernova remnant
• A Survey of Magnetic Field Strengths in the Envelopes of Molecular Clouds via the 18 cm OH Zeeman Effect
• Multifluid magnetohydrodynamic turbulent decay
• Kinetic and internal energy transfer in implicit large eddy simulations of forced compressible turbulence
• Turbulence and Accretion: a High-resolution Study of the B5 Filaments
• HII regions and high-mass starless clump candidates I: Catalogs and properties
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy
• 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
• Filamentary Star Formation: Observing the Evolution toward Flattened Envelopes
• The Column Density Variance in Turbulent Interstellar Media: A Fractal Model Approach
• MRI-driven angular momentum transport in protoplanetary disks
• The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS)
• Universal gravity-driven isothermal turbulence cascade in disk galaxies
• Infall, outflow, and turbulence in massive star-forming cores in the G333 giant molecular cloud
• Observations of chemical differentiation in clumpy molecular clouds
• The JCMT Gould Belt Survey: Understanding the influence of molecular outflows on Gould Belt clouds
• Modelling the structure of molecular clouds: I. A multi-scale energy equipartition
• The Nature of Turbulence in the LITTLE THINGS Dwarf Irregular Galaxies
• Large-scale turbulent driving regulates star formation in high-redshift gas-rich galaxies II: Influence of the magnetic field and the turbulent compressive fraction
• Star formation in Chamaeleon I and III: a molecular line study of the starless core population
• Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification
• Cloud Dispersal in Turbulent Flows
• Turbulence decay and cloud core relaxation in molecular clouds
• Clump mass function at an early stage of molecular cloud evolution: I. A statistical approach
• Toward Understanding the Origin of Turbulence in Molecular Clouds: Small Scale Structures as Units of Dynamical Multi-Phase Interstellar Medium
• Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC7674
• A Force Explosion Condition for Spherically Symmetric Core-collapse Supernovae
• Dynamo effect in unstirred self-gravitating turbulence
• Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence
• Gravitational Fragmentation of Extremely Metal-poor Circumstellar Discs
• The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 star-forming Clump
• Non-ideal MHD turbulent decay in molecular clouds
• Quiescent Isolation: The Extremely Extended HI Halo of the Optically Compact Dwarf Galaxy ADBS 113845+2008
• Intermittency of Fast MHD Modes and Regions of Anomalous Gradient Orientation in Low-beta Plasmas
• A Search for correlations between turbulence and star formation in THINGS galaxies
• Magnetic Field Strengths in Photodissociation Regions
• TIMES I: a Systematic Observation in Multiple Molecular Lines Toward the Orion A and Ophiuchus Clouds
• 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
• 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
• Dependence of the Star Formation Efficiency on the Parameters of Molecular Cloud Formation Simulations
• High-resolution HI and CO observations of high-latitude intermediate-velocity clouds
• Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence
• Implementing and comparing sink particles in AMR and SPH
• Probing Turbulence with Infrared Observations in OMC1
• Structure analysis of simulated molecular clouds with the Delta-variance
• Type III Societies (Apparently) Do Not Exist
• Radiation feedback in dusty clouds
• Distortion of Magnetic Fields in a Starless Core VI: Application of Flux Freezing Model and Core Formation of FeSt 1-457
• Census of Gaseous Satellites around Local Spiral Galaxies
• Simulated observations of star formation regions: infrared evolution of globally collapsing clouds
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Spectroscopic Confirmation of a Population of Isolated, Intermediate-Mass YSOs
• On filament fragmentation and the impact of ambient environment on it
• The magnetic field in the dense photodissociation region of DR 21
• Necessary conditions for the formation of filaments and star clusters in the cold neutral medium
• Magnetic Flux Transport by turbulent reconnection in astrophysical flows
• Gravity or turbulence V: Star forming regions undergoing violent relaxation
• A Dynamically Collapsing Core and a Precursor of a Core in a Filament Supported by Turbulent and Magnetic Pressures
• Starbursts and High-Redshift Galaxies are Radioactive: High Abundances of ${}^{26}$Al and Other Short Lived Radionuclides
• Characterization of Turbulence from Submillimeter Dust Emission
• Cloud properties across spatial scales in simulations of the interstellar medium
• Generation of Solenoidal Modes and Magnetic Fields in Turbulence Driven by Compressive Driving
• Galactic Magnetic Turbulence from Radio data
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
• Assessing the Impact of Astrochemistry on Molecular Cloud Turbulence Statistics
• Bipolar molecular outflow of the very low-mass star Par-Lup3-4
• Interstellar Turbulence and Star Formation
• The Interstellar Medium and Star Formation in Local Galaxies: Variations of the Star Formation Law in Simulations
• Number ratios of young stellar objects in embedded clusters
• The evolution of the internal structure of massive star forming regions in the Milky Way as revealed by ALMA
• Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds
• Observational studies of pre-stellar cores and infrared dark clouds
• A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its variation on redshift and stellar mass
• Inefficient star formation in high Mach number environments I. The turbulent support analytical model
• CO-0.30-0.07: A Peculiar Molecular Clump with an Extremely Broad Velocity Width
• Formation of metal-free binaries: Impact of H${}_2$ line cooling and CIE cooling
• Linear dust polarization during the embedded phase of protostar formation
• Numerical Simulations of a Protostellar Outflow Colliding with a Dense Molecular Cloud
• Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde V. The massive filament DR21
• Simulations of pre-supernova feedback in spherical clouds
• Low-Mass Star Forming Cores in the GF9 Filament
• Testing assumptions and predictions of star-formation theories
• The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
• Compact dusty clouds and efficient H${}_2$ formation in diffuse ISM
• Centrally concentrated molecular gas driving galactic-scale ionised gas outflows in star-forming galaxies
• Interactions of a shock with a molecular cloud at various stages of its evolution due to thermal instability and gravity
• Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
• The kinetic and magnetic energy budget of hub-filament systems during the gravitational fragmentation of molecular clouds
• Density and Velocity Correlations in Isothermal Supersonic Turbulence
• Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• Gradient measurement of synchrotron polarization diagnostic: Application to spatially separated emission and Faraday rotation regions
• DIISC-II: Unveiling the Connections between Star Formation and ISM in the Extended Ultraviolet Disk of NGC 3344
• CN Zeeman observations of the NGC 2264-C protocluster
• Photoionization feedback in turbulent molecular clouds
• OH maser toward IRAS 06056+2131: polarization parameters and evolution status
• Chaotic behavior of Eulerian MHD turbulence
• Synthetic Observations of Carbon Lines of Turbulent Flows in Diffuse Multiphase Interstellar Medium
• Can the removal of molecular cloud envelopes by external feedback affect the efficiency of star formation?
• Nonlinear Criterion for the Stability of Molecular Clouds
• 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
• From Gas to Stars Over Cosmic Time
• On the Functional Form of the Universal Star Formation Law
• Characterizing star formation activity in infrared dark cloud MSXDC G048.65-00.29
• An ALMA search for substructure and fragmentation in starless cores in Orion B North
• The influence of the cloud virial parameter on the initial mass function
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS
• Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
• The Spatial Power Spectrum and Derived Turbulent Properties of Isolated Galaxies
• Shocked Molecular Hydrogen and Broad CO lines from the Interacting Supernova Remnant HB 3
• Explosion Energies for Core-collapse Supernovae I: Analytic, Spherically Symmetric Solutions
• IRAS 09002-4732: A Laboratory for the Formation of Rich Stellar Clusters
• Statistical properties and correlation length in star-forming molecular clouds: I. Formalism and application to observations
• Star Formation at the Galactic Center
• Evolution of gaseous disk viscosity driven by supernova explosion. II. Structure and emissions from star-forming galaxies at high redshift
• Simultaneously modelling far-infrared dust emission and its relation to CO emission in star forming galaxies
• 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
• ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump
• Characterization of a turbulent flow with independent variation of Mach and Reynolds numbers
• A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
• Open questions in the study of population III star formation
• Hubble-Lemaître fragmentation and the path to equilibrium of merger-driven cluster formation
• Molecular Line Profiles from a Core Forming in a Turbulent Cloud
• Formation of the First Galaxies: Theory and Simulations
• The Degeneracy of Galaxy Formation Models
• Multiwavelength Studies of Young OB Associations
• Initial Ionization of Compressible Turbulence
• Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
• Scales of Stability and Turbulence in the Molecular ISM
• Differences in chemical evolution between isolated and embedded prestellar cores
• Density Exponent Analysis: Gravity-driven steepening of the density profiles of star-forming regions
• 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
• Fragmentation and Structure Formation
• 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
• The High Rate of the Boyajian's Star Anomaly as a Phenomenon
• Theories of the initial mass function
• Turbulence and its connection to episodic accretion in binary YSOs
• Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
• Mean fields and fluctuations in compressible magnetohydrodynamic flows
• Inefficient star formation in high Mach number environments II. Numerical simulations and comparison with analytical models
• Deviation from a Continuous and Universal Turbulence Cascade in NGC 6334 due to Massive Star Formation Activity
• Formation of low-mass stars and brown dwarfs
• The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
• Turbulence driven by stellar jets, the possibility and the efficiency
• Powerful flare phenomena in water vapor maser lines in the emerging protostellar system with protoplanetary disks IRAS 16293-2422
• Reconstructing the genesis of a globular cluster system at a look-back time of 9.1 Gyr with the JWST
• Dynamic duos: the building blocks of dimensional mechanics
• The magnetic field in the Flame nebula
• Massive star cluster formation III. Early mass segregation during cluster assembly
• 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
• Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
• A Deep Neural Network Approach to Compact Source Removal
• The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Rubin LSST observing strategies to maximize volume and uniformity coverage of Star Forming Regions in the Galactic Plane
• Relative Alignment Between Magnetic Fields and Molecular Gas Structure in Molecular Clouds
• Line emission from filaments in molecular clouds
• Star-forming environments in smoothed particle magnetohydrodynamics simulations I: Clump extraction and properties
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Finite shock model of density in supersonic turbulence
• Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences
• Studying Interstellar Turbulence Driving Scales using the Bispectrum
• The turbulence driving parameter of molecular clouds in disc galaxies
• The formation, disruption and properties of pressure-supported stellar systems and implications for the astrophysics of galaxies
• Studying the properties of compressible MHD turbulence by synchrotron fluctuation statistics
• 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${}^{\circ }$
• Simulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs
• Studies of Dense Cores with ALMA
• Late encounter-events as a source of disks and spiral structures -- Forming second generation disks
• Dust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains
• Impact of radiation feedback on the assembly of star clusters in galactic context
• Spiral arm triggering of star formation
• Density profile of a self-gravitating polytropic turbulent fluid in a rotating disk near to the cloud core
• Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
• Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions
• The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
• Rydberg States of H${}_3$ and HeH as Potential Coolants for Primordial Star Formation
• Power spectra of outflow-driven turbulence
• Inverse Hubble Flows in Molecular Clouds
• Anisotropy of Magnetohydrodynamic Turbulence and Polarization of the Spectral Lines of Molecules
• Examining Turbulence in Galactic Molecular Clouds -- I: A Statistical Analysis of Velocity Structures
• Turbulent Control of the Star Formation Efficiency
• Deuterium fractionation of the starless core L 1498
• Can galactic magnetic fields diffuse into the voids?
• Structure of iso-density sets in supersonic isothermal turbulence
• Magnetic fields and hot gas in M101
• Measuring Young Stars in Space and Time -- I. The Photometric Catalog and Extinction Properties of N44
• The kinematics of the magnetised protostellar core IRAS15398-3359
• The Turbulent Interstellar Medium: Insights and Questions from Numerical Models
• Obtaining strength of magnetic field from E and B modes of dust polarization
• Turbulence in the Star-forming Interstellar Medium: Steps toward Constraining Theories with Observations
• On the role of stochastic Fermi acceleration in setting the dissipation scale of turbulence in the interstellar medium
• From Gas to Stars over Cosmic Time
• Measurement of the scaling slope of compressible magnetohydrodynamic turbulence by synchrotron radiation statistics
• Molecular Fluctuations Inhibit Intermittency in Compressible Turbulence
• Modeling the Disk (three-phase) Interstellar Medium
• Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
• Understanding the IMF
• A Search for 3-mm Molecular Absorption Line Transitions in the Magellanic Stream
• Statistical signatures of interstellar turbulence in dust polarization maps
• A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity
• Measuring the spectral index of turbulent gas with deep learning from projected density maps
• Simulations of the IMF in Clusters
• Numerical Methods for Simulating Star Formation
• Young massive star clusters: Achievements and challenges
• Sound-Triggered Collapse of Stably Oscillating Low-Mass Cores in a Two-Phase Interstellar Medium
• Chemical chronology of the Southern Coalsack
• Parallel and Perpendicular Alignments of Velocity Gradient and Magnetic Field observed in the Molecular Clouds L1478 and L1482
• Prospects of Turbulence Studies in High-Energy Density Laser-Generated Plasma: Numerical Investigations in Two Dimensions
• Thermal damping of Weak Magnetosonic Turbulence in the Interstellar Medium
• A photo-ionized canopy for the shock-excited Criss-Cross Nebula
• Hydrodynamic and Magnetohydrodynamic Simulations of Wire Turbulence
• Stable smoothed particle magnetohydrodynamics in very steep density gradients
• Cloud fragmentation cascades and feedback: on reconciling an unfettered inertial range with a low star formation rate
• Molecular Cloud Turbulence And The Star Formation Efficiency: Enlarging the Scope
• A method for detection of structure
• Magnetic Fields Studies in the Next Decade: EAO Submillimetre Futures White Paper Series, 2019
• Observations of Protostellar Outflow Feedback in Clustered Star Formation
• Formation of star-forming clouds from the magnetised, diffuse interstellar medium
• Estimating the dense gas mass of molecular clouds using spatially unresolved 3 mm line observations
• Primordial Black Holes Formed during Magneto-Hydrodynamic Turbulence in The Early Universe as Dominant Part of Dark Matter
• Collapsing Index: A New Method to Identify Star-forming Cores Based on ALMA Images
• On the interaction of a thin, supersonic shell with a molecular cloud
• Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
• The Supernova-ISM/Star formation Interplay
• Intermittency and non-universality of pair dispersion in isothermal compressible turbulence
• Cluster Density and the IMF
• Supernova origin of galactic turbulence revealed by superbubbles
• Turbulence in the Molecular Interstellar Medium
• Thermal instability through the outer half of quasi-static spherically symmetric molecular clumps and cores
• The Numerical Simulation of Turbulence
• The interdependence between density PDF, CMF and IMF and their relation with Mach number in simulations
• Dynamical Evolution of a Supernova Driven Turbulent Interstellar Medium
• A localized dynamic closure model for Euler turbulence
• Magnetic fields in star forming environments: how does field strength affect gas on spiral arm and cloud scales?
• Power spectrum to probe turbulence in Interstellar medium using 21cm line
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
• Cosmic Ray Propagation in Turbulent Spiral Magnetic Fields associated with Young Stellar Objects
• On the structure of giant HII regions and HII galaxies
• Shock fragmentation model for gravitational collapse
• Time Variability in Simulated Ultracompact and Hypercompact HII Regions
• (Sub)mm Interferometry Applications in Star Formation Research
• From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data
• NH3 (1,1) hyperfine intensity anomalies in infall sources
• Mass Segregation in the CMZoom Survey
• Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
• The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics
• CO Structures with Narrow Lines in Nearby Quiescent Regions
• Vortex Detection from Quantum Data
• Heavy interstellar scattering toward the near end of the Galactic bar
• A resolution criterion based on characteristic timescales for MHD simulations of molecular clouds
• Self-confinement of low-energy cosmic rays around supernova remnants
• 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
• On the star formation rate and turbulent dissipation in galactic models
• Environmental Effects on the Dynamical Evolution of Star Clusters in Turbulent Molecular Clouds
• On the scale-height of the molecular gas disc in Milky Way-like galaxies
• The signature of large scale turbulence driving on the structure of the interstellar medium
• Supernovae and photoionizing feedback in spiral arm molecular clouds
• Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes
• Why most molecular clouds are gravitationally dominated
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies