Interstellar Turbulence I: Observations and Processes

Abstract

This two-part review summarizes interstellar turbulence and its implications. The first part begins with diagnostics and energy sources. Turbulence theory is considered in detail, including the basic fluid equations, solenoidal and compressible modes, global inviscid quadratic invariants, scaling arguments, energy transfer and cascade, velocity probability distributions, and turbulent pressure. Theories of magnetohydrodynamic turbulence, including collisionless MHD turbulence, are discussed, emphasizing various proposals for energy spectra. A large variety of numerical simulations of interstellar turbulence are reviewed. Models have reproduced many of the basic features of the observed scaling relations, predicted fast decay rates for supersonic MHD turbulence, and derived probability distribution functions for density. Thermal instabilities and thermal phases have a new interpretation in a turbulent medium. Large-scale models with various combinations of self-gravity, magnetic fields, supernovae, and star formation are beginning to resemble the observed interstellar medium in morphology and statistical properties. The role of self-gravity in turbulent gas is clarified, leading to new paradigms for the formation of star clusters, the stellar mass function, the origin of stellar rotation and binary stars, and the effects of magnetic fields.

71 pages, 5 figures, submitted to Annual Reviews of Astronomy and Astrophysics

References in corpus (3)

• Is nonhelical hydromagnetic turbulence peaked at small scales?
• Effects of forcing in three dimensional turbulent flows
• The decay of homogeneous anisotropic turbulence

Cited by in corpus (778)

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• Cold Dark Clouds: The Initial Conditions for Star Formation
• Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
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• A primer on hierarchical galaxy formation: the semi-analytical approach
• The Resolved Properties of Extragalactic Giant Molecular Clouds
• The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• The Local Dark Matter Density
• On the fraction of star formation occurring in bound stellar clusters
• Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
• Tracing Magnetic Fields with Aligned Grains
• Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH
• Science with ASKAP - the Australian Square Kilometre Array Pathfinder
• On the Star Formation Efficiency of Turbulent Magnetized Clouds
• Global Hierarchical Collapse In Molecular Clouds. Towards a Comprehensive Scenario
• Numerical Tests of Fast Reconnection in Weakly Stochastic Magnetic Fields
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• What is Driving the HI Velocity Dispersion?
• Dissipation of Magnetohydrodynamic Waves on Energetic Particles: Impact on Interstellar Turbulence and Cosmic Ray Transport
• The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
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• Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
• On the universality of supersonic turbulence
• Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
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• The driving mechanism of starbursts in galaxy mergers
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• Inefficient star formation through turbulence, magnetic fields and feedback
• Protostellar Turbulence Driven by Collimated Outflows
• Gravity or Turbulence? The velocity dispersion-size relation
• Extending Big Power Law in the Sky with Turbulence Spectra from WHAM data
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• Cosmic Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field
• Formation of Massive Molecular Cloud Cores by Cloud-cloud Collision
• Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas
• The Birth of High Mass Stars: Accretion and/or Mergers?
• Magnetic Fields in Dark Cloud Cores: Arecibo OH Zeeman Observations
• The Fractal Density Structure in Supersonic Isothermal Turbulence: Solenoidal versus Compressive Energy Injection
• The supernova rate-velocity dispersion relation in the interstellar medium
• The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows
• Tidally Heated Terrestrial Exoplanets: Viscoelastic Response Models
• The Atlas3D Project - VI. Simulations of binary galaxy mergers and the link with Fast Rotators, Slow Rotators, and Kinematically Distinct Cores
• Three Dimensional Hydrodynamic Simulations of Multiphase Galactic Disks with Star Formation Feedback: I. Regulation of Star Formation Rates
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• Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum
• Exact relation for correlation functions in compressible isothermal turbulence
• 3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications
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• Importance of the Initial Conditions for Star Formation - I. Cloud Evolution and Morphology
• Herschel-SPIRE observations of the Polaris flare : structure of the diffuse interstellar medium at the sub-parsec scale
• Modeling jet and outflow feedback during star cluster formation
• The Relationship Between Molecular Gas Tracers and Kennicutt-Schmidt Laws
• Partially Ionized Plasmas in Astrophysics
• The Stellar IMF, Core Mass Function, & The Last-Crossing Distribution
• Velocity Field of Compressible MHD Turbulence: Wavelet Decomposition and Mode Scalings
• A robust numerical scheme for highly compressible magnetohydrodynamics: Nonlinear stability, implementation and tests
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• The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim 2.6$ to $z\sim 0.6$ with KMOS${}^{3D}$
• Dependence of Interstellar Turbulent Pressure on Supernova Rate
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• Modelling CO formation in the turbulent interstellar medium
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• Dynamical Expansion of Ionization and Dissociation Front around a Massive Star. II. On the Generality of Triggered Star Formation
• On the evolution of the density pdf in strongly self-gravitating systems
• Chains of dense cores in the Taurus L1495/B213 complex
• Powerful High Velocity-Dispersion Molecular Hydrogen Associated with an Intergalactic Shock Wave in Stephan's Quintet
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• Molecular Cloud Evolution IV: Magnetic Fields, Ambipolar Diffusion, and the Star Formation Efficiency
• A General Theory of Turbulent Fragmentation
• Magnetic field amplification in turbulent astrophysical plasmas
• Exact Relation with Two-point Correlation Functions and Phenomenological Approach for Compressible Magnetohydrodynamic Turbulence
• On the nature of star-forming filaments: II. Sub-filaments and velocities
• How supernova explosions power galactic winds
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• DYNAMO I: A Sample of Ha-Luminous Galaxies with Resolved Kinematics
• Characterizing Magnetohydrodynamic Turbulence in the Small Magellanic Cloud
• A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey
• The link between molecular cloud structure and turbulence
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• SILCC-Zoom: The dynamical and chemical evolution of molecular clouds
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• Turbulence-induced magnetic fields and the structure of Cosmic Ray modified shocks
• Astrophysical hydromagnetic turbulence
• Dynamical HII Region Evolution in Turbulent Molecular Clouds
• Chaotic cold accretion on to black holes in rotating atmospheres
• The Global Evolution of Giant Molecular Clouds II: The Role of Accretion
• Large scale galactic turbulence: can self-gravity drive the observed HI velocity dispersions?
• Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
• The Southern Galactic Plane Survey: Polarized Radio Continuum Observations and Analysis
• Six Myths on the Virial Theorem for Interstellar Clouds
• SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium
• Testing Magnetic Star Formation Theory
• Star Cluster Formation in Turbulent, Magnetized Dense Clumps with Radiative and Outflow Feedback
• Quiescent Cores and the Efficiency of Turbulence-Accelerated, Magnetically Regulated Star Formation
• The formation of molecular clouds in spiral galaxies
• The interplay between chemical and mechanical feedback from the first generation of stars
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• Studying Turbulence using Doppler-broadened lines: Velocity Coordinate Spectrum
• Velocity Gradients as a Tracer for Magnetic Fields
• Superdiffusion of Cosmic Rays: Implications for Cosmic Ray Acceleration
• Turbulence, Magnetic Reconnection in Turbulent Fluids and Energetic Particle Acceleration
• The Generation and Dissipation of Interstellar Turbulence - Results from Large Scale High Resolution Simulations
• A model of acceleration of Anomalous Cosmic Rays by Reconnection in the Heliosheath
• Vertical Equilibrium, Energetics, and Star Formation Rates in Magnetized Galactic Disks Regulated by Momentum Feedback from Supernovae
• The Virial Balance of Clumps and Cores in Molecular Clouds
• The density structure and star formation rate of non-isothermal polytropic turbulence
• Hierarchical Star Formation in the Spiral Galaxy NGC 628
• A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence
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• The Formation of the First Stars in the Universe
• Adiabatic Heating of Contracting Turbulent Fluids
• A new density variance - Mach number relation for subsonic and supersonic, isothermal turbulence
• Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
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• The spatial distribution of stars in open clusters
• Obtaining Spectra of Turbulent Velocity from Observations
• On the von Karman-Howarth equations for Hall MHD flows
• Velocity Spectrum for HI at High Latitudes
• Statistical Description of Synchrotron Intensity Fluctuations: Studies of Astrophysical Magnetic Turbulence
• SPICY: The Spitzer/IRAC Candidate YSO Catalog for the Inner Galactic Midplane
• Generation of Magnetic Fields in the Multi-phase ISM with Supernova-Driven Turbulence
• The Magnetohydrodynamics of Shock-Cloud Interaction in Three Dimensions
• Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse
• Algorithmic comparisons of decaying, isothermal, supersonic turbulence
• A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces: I. Cloud-scale Gas Motions
• Studying Galactic interstellar turbulence through fluctuations in synchrotron emission: First LOFAR Galactic foreground detection
• Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
• Gas expulsion in massive star clusters? Constraints from observations of young and gas-free objects
• The Musca cloud: A 6 pc-long velocity-coherent, sonic filament
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• Evolution of supernovae-driven superbubbles with conduction and cooling
• Feeding SMBHs through supersonic turbulence and ballistic accretion
• Angular Momentum Transfer and Lack of Fragmentation in Self-Gravitating Accretion Flows
• Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
• 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
• Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scale
• Ionization compression impact on dense gas distribution and star formation, Probability density functions around H ii regions as seen by Herschel
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• Intermittency and Universality in Fully-Developed Inviscid and Weakly-Compressible Turbulent Flows
• The Spatial Relation between Young Star Clusters and Molecular Clouds in M 51 with LEGUS
• A supersonic turbulence origin of Larson's laws
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• Dissecting the IRX - $\beta$ dust attenuation relation: exploring the physical origin of observed variations in galaxies
• New Tests for Disruption Mechanisms of Star Clusters: Methods and Application to the Antennae Galaxies
• Feedback Effects on Low-Mass Star Formation
• Turbulence driven by outflow-blown cavities in the molecular cloud of NGC 1333
• Chaos and Variance in Galaxy Formation
• Molecules in galaxies
• Enhanced small-scale Faraday rotation in the Galactic spiral arms
• Supersonic turbulence, filamentary accretion,and the rapid assembly of massive stars and disks
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• Magnetohydrodynamic turbulence mediated by reconnection
• The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds
• Thermal-Instability-Driven Turbulent Mixing in Galactic Disks: I. Effective Mixing of Metals
• Millimeter-Wave Line Ratios and Sub-beam Volume Density Distributions
• Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation
• Astrophysical turbulence modeling
• Role of the Plasmoid Instability in Magnetohydrodynamic Turbulence
• Magnetization of cloud cores and envelopes and other observational consequences of reconnection diffusion
• Density Profiles in Seyfert Outflows
• A common solution to the cosmic ray anisotropy and gradient problems
• A closer look at the "characteristic" width of molecular cloud filaments
• Plasmoid Instability in Forming Current Sheets
• GaussPy+: A fully automated Gaussian decomposition package for emission line spectra
• Spectrum and Anisotropy of Turbulence from Multi-Frequency Measurement of Synchrotron Polarization
• Dynamical and Spectral Modeling of the Ionized Gas and Nuclear Environment in NGC 3783
• The conservative cascade of kinetic energy in compressible turbulence
• The origin of physical variations in the star formation law
• The structure of the thermally bistable and turbulent atomic gas in the local interstellar medium
• Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
• Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments
• A Toomre-like stability criterion for the clumpy and turbulent interstellar medium
• SCUBA and Spitzer observations of the Taurus molecular cloud - pulling the bull's tail
• Opacity broadening and interpretation of suprathermal CO linewidths: Macroscopic Turbulence and Tangled Molecular Clouds
• Disruption of Molecular Clouds by Expansion of Dusty H II Regions
• Cold Milky Way Hi gas in filaments
• Gravitational Runaway and Turbulence Driving in Star-Gas Galactic Disks
• On the self-regulation of intense star-formation in galaxies at z=1-3
• Ultrafaint Dwarf Galaxies - the lowest mass relics from before reionization
• Physical Processes in Star Formation
• Cloud and Star Formation in Disk Galaxy Models with Feedback
• The Matryoshka Run: Eulerian Refinement Strategy to Study Statistics of Turbulence in Virialized Cosmic Structures
• Scaling Relations of Compressible MHD Turbulence
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• Saturation of the Turbulent Dynamo
• Radioactive 26Al from the Scorpius-Centaurus Association
• Outflow Driven Turbulence in Molecular Clouds
• The structure and statistics of interstellar turbulence
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• Observational Diagnostics of Self-Gravitating MHD Turbulence in Giant Molecular Clouds
• The turbulent formation of stars
• Turbulence in the Interstellar Medium
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• The turbulent destruction of clouds - I. A k-epsilon treatment of turbulence in 2D models of adiabatic shock-cloud interactions
• From diffuse gas to dense molecular cloud cores
• Distribution of velocity gradient orientations: Mapping magnetization with the Velocity Gradient Technique
• Dust and gas power-spectrum in M33 (HERM33ES)
• Damping of Alfven waves by Turbulence and its Consequences: from Cosmic-Rays Streaming to Launching Winds
• The Complex Distribution of Recently Formed Stars. Bimodal Stellar Clustering in the Star-Forming Region NGC 346
• Properties of Interstellar Turbulence from Gradients of Linear Radio Polarization Maps
• CARMA Large Area Star Formation Survey: Structure and Kinematics of Dense Gas in Serpens Main
• Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
• Reconnection Studies Under Different Types of Turbulence Driving
• Density probability distribution functions of diffuse gas in the Milky Way
• Pressure Support in Galaxy Disks: Impact on Rotation Curves and Dark Matter Density Profiles
• The Spatial Distribution of the Young Stellar Clusters in the Star Forming Galaxy NGC 628
• The Physical Nature of Neutral Hydrogen Intensity Structure
• Structure of Stationary Strong Imbalanced Turbulence
• The SILCC project - V. The impact of magnetic fields on the chemistry and the formation of molecular clouds
• Energisation of interstellar media and cosmic ray production by jets from X-ray binaries
• Evolution of Magnetic Fields in High Mass Star Formation: SMA dust polarization image of the UCHII region G5.89-0.39
• von Kármán energy decay and heating of protons and electrons in a kinetic turbulent plasma
• Can Protostellar Jets Drive Supersonic Turbulence in Molecular Clouds?
• Critical Balance and the Physics of MHD Turbulence
• Structure analysis of interstellar clouds: I. Improving the Delta-variance method
• Unbound Young Stellar Systems: Star Formation on the loose
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: I. Turbulence Statistics
• Plasma turbulence in the interstellar medium
• On the effect of cosmological inflow on turbulence and instability in galactic discs
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• Studying Turbulence from Doppler-broadened Absorption Lines: Statistics of Logarithms of Intensity
• M82, Starbursts, Star Clusters, and the Formation of Globular Clusters
• Dark cloud cores and gravitational decoupling from turbulent flows
• Star formation in turbulent molecular clouds with colliding flow
• Formation of slowly rotating early-type galaxies via major mergers: a Resolution Study
• Power spectrum of HI intensity fluctuations in DDO 210
• The Turbulence Power Spectrum in Optically Thick Interstellar Clouds
• Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing
• A Study of ISM of Dwarf Galaxies Using HI Power Spectrum Analysis
• Adaptive Mesh Refinement for Supersonic Molecular Cloud Turbulence
• Development of Anisotropy in Incompressible Magnetohydrodynamic Turbulence
• The Turbulence Velocity Power Spectrum of Neutral Hydrogen in the Small Magellanic Cloud
• The Elongations and Supersonic Motions of Molecular Clouds
• What drives gravitational instability in nearby star-forming spirals? The impact of CO and HI velocity dispersions
• Constraints on the ICM velocity power spectrum from the X-ray lines width and shift
• Classification of Filament Formation Mechanisms in Magnetized Molecular Clouds
• 129I and 247Cm in Meteorites Constrain the Last Astrophysical Source of Solar r-process Elements
• 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
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• Measuring the Alfvenic Nature of the Interstellar Medium: Velocity Anisotropy Revisited
• 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
• Surviving infant mortality in the hierarchical merging scenario
• Hierarchical Structure of Magnetohydrodynamic Turbulence In Position-Position-Velocity Space
• Systematics of the magnetic-Prandtl-number dependence of homogeneous, isotropic magnetohydrodynamic turbulence
• Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields
• 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
• Turbulent dynamo in the two-phase interstellar medium
• From primordial seed magnetic fields to the galactic dynamo
• Observability of the very-high-energy emission from GRB 221009A
• The Nonisothermal Stage of Magnetic Star Formation. I. Formulation of the Problem and Method of Solution
• Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
• Spitzer Space Telescope observations of the Carina Nebula: The steady march of feedback-driven star formation
• Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
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• Vortices in the wakes of AGB stars
• Particle acceleration in strong MHD turbulence
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• 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
• An Evolutionary Model for Collapsing Molecular Clouds and Their Star Formation Activity. II. Mass Dependence of the Star Formation Rate
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• Nature of the Wiggle Instability of Galactic Spiral Shocks
• Superdiffusion of Cosmic Rays in Compressible Magnetized Turbulence
• Characterizing gravitational instability in turbulent multi-component galactic discs
• A Two-Component Power Law Covering Nearly Four Orders of Magnitude in the Power Spectrum of Spitzer Far-Infrared Emission from the Large Magellanic Cloud
• Molecular and Atomic Gas in the Large Magellanic Cloud - I. Conditions for CO Detection
• Beyond the nuclear starburst? Clustered star formation in major mergers
• Test particle simulations of cosmic rays
• The Small-Scale Dynamo at Low Magnetic Prandtl Numbers
• Interstellar Turbulence Driving by Galactic Spiral Shocks
• Cosmic rays in galactic and extragalactic magnetic fields
• Atomic and Ionized Microstructures in the Diffuse Interstellar Medium
• The strength and structure of the magnetic field in the galactic outflow of M82
• On the Evolution of the Dense Core Mass Function
• Forced turbulence in thermally bistable gas: A parameter study
• The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• Is molecular cloud turbulence driven by external supernova explosions?
• Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence
• A Kolmogorov-Like Exact Relation for Compressible Polytropic Turbulence
• Galactic interstellar turbulence in the southern sky seen through spatial gradients of the polarization vector
• Alfvenic Turbulence Beyond the Ambipolar Diffusion Scale
• A Case Study of Low-Mass Star Formation
• CARMA Large Area Star Formation Survey: Project Overview with Analysis of Dense Gas Structure and Kinematics in Barnard 1
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Interstellar Sonic and Alfvénic Mach Numbers and the Tsallis Distribution
• The initial mass function of star clusters that form in turbulent molecular clouds
• Densities and filling factors of the DIG in the Solar neighbourhood
• The turbulent destruction of clouds - III. Three dimensional adiabatic shock-cloud simulations
• Dust polarization and ISM turbulence
• Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code
• The role of magnetic fields in the structure and interaction of supershells
• Shock Waves and Energy Dissipation in Magnetohydrodynamic Turbulence
• Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
• HI Power Spectra and the Turbulent ISM of Dwarf Irregular Galaxies
• Geophysical-astrophysical spectral-element adaptive refinement (GASpAR): Object-oriented h-adaptive code for geophysical fluid dynamics simulation
• Plasma Diagnostics of the Interstellar Medium with Radio Astronomy
• A switch to reduce resistivity in smoothed particle magnetohydrodynamics
• Viriato: a Fourier-Hermite spectral code for strongly magnetised fluid-kinetic plasma dynamics
• The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
• Turbulence in the outer heliosphere
• On the shape and completeness of the column density probability distribution function of molecular clouds
• The Scale Height of NGC 1058 Measured from its HI Power Spectrum
• Classification of Magnetohydrodynamic Simulations using Wavelet Scattering Transforms
• Energy budget of forming clumps in numerical simulations of collapsing clouds
• HI power spectrum of the spiral galaxy NGC628
• GASKAP-HI Pilot Survey Science I: ASKAP Zoom Observations of HI Emission in the Small Magellanic Cloud
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Interpreting the sub-linear Kennicutt-Schmidt relationship: The case for diffuse molecular gas
• Hierarchical Stellar Structures in the Local Group Dwarf Galaxy NGC 6822
• Time-dependent perpendicular transport of fast charged particles in a turbulent magnetic field
• The Multi-phase Turbulence Density Power Spectra in the Perseus Molecular Cloud
• Looking for MACHOs in the Spectra of Fast Radio Bursts
• A Statistical Investigation of HI in the Magellanic Bridge
• Shock interactions, turbulence, and the origin of the stellar mass spectrum
• Star Formation in Molecular Clouds
• Physical Properties of Complex C Halo Clouds
• Constraining the Earliest Circumstellar Disks and their Envelopes
• Study of velocity centroids based on the theory of fluctuations in position-position-velocity space
• Synthetic observations of star formation and the interstellar medium
• The Efficiency of Magnetic Field Amplification at Shocks by Turbulence
• The Fractal Distribution of HII Regions in Disk Galaxies
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• Three-dimensional extinction mapping using Gaussian random fields
• Magnetized Non-linear Thin Shell Instability: Numerical Studies in 2D
• Jet Formation in 3D GRMHD Simulations of Bondi-Hoyle-Lyttleton Accretion
• IRAM-30m large scale survey of ${}^{12}$CO(2-1) and ${}^{13}$CO(2-1) emission in the Orion molecular cloud
• Local Star formation triggered by SN shocks in magnetized diffuse neutral clouds
• The effect of ISM turbulence on the gravitational instability of galactic discs
• VLBA observations of a rare multiple quasar imaging event caused by refraction in the interstellar medium
• Simulations of cosmic ray propagation
• Magnetic field strength from turbulence theory (I): Using differential measure approach (DMA)
• The bispectrum of polarized galactic foregrounds
• The Power Spectra of Polarized, Dusty Filaments
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• Role of reconnection in inertial kinetic-Alfven turbulence
• Interaction of Jets with the ISM of Radio Galaxies
• 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
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• TurbuStat: Turbulence Statistics in Python
• Local Turbulence Simulations for the Multiphase ISM
• Clumpy and fractal shocks, and the generation of a velocity dispersion in molecular clouds
• Properties of the Magneto-ionic Medium in the Halo of M51 revealed by Wide-band Polarimetry
• Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies
• Cosmic Ray transport through gyroresonance instability in compressible turbulence
• The metallicity of galactic winds
• Fine Structures of Solar Radio Type III Bursts and their Possible Relationship with Coronal Density Turbulence
• Velocity Gradient in the Presence of Self-Gravity: Identifying Gravity-induced Inflow and Determining Collapsing Stage
• Mach number study of supersonic turbulence: The properties of the density field
• Identification of plasma modes in Galactic turbulence with synchrotron polarization
• The Origin of Interstellar Turbulence in M33
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Interstellar cloud structure: The statistics of centroid velocities
• Shock generated vorticity in the interstellar medium and the origin of the stellar initial mass function
• Efficiency of metal mixing in dwarf galaxies
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. I. The unmagnetized and zero-feedback limit
• Structure analysis of interstellar clouds: II. Applying the Delta-variance method to interstellar turbulence
• Fast Magnetic Reconnection and Energetic Particle Acceleration
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• Multifractal Analysis of the Interstellar Medium. First application to Hi-GAL Observations
• Damping of MHD turbulence in partially ionized gas and the observed difference of velocities of neutrals and ions
• The properties of SCUBA cores in the Perseus molecular cloud: the bias of clump-finding algorithms
• The VMC Survey. XXIX. Turbulence-Controlled Hierarchical Star Formation in the Small Magellanic Cloud
• Shock-multicloud interactions in galactic outflows -- I. Cloud layers with log-normal density distributions
• A Simple Perspective on the Mass-Area Relationship in Molecular Clouds
• The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas
• The Turbulent Interstellar Medium
• MHD Turbulence, Turbulent Dynamo and Applications
• On the turbulence driving mode of expanding HII regions
• PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA
• The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence
• Flux Correlations in Supersonic Isothermal Turbulence
• On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies
• The Kelvin-Helmholtz instability in Orion: a source of turbulence and chemical mixing
• Power Spectra in V-band and Halpha of Nine Irregular Galaxies
• Compressible turbulence in the interstellar medium: New insights from a high-resolution supersonic turbulence simulation
• Turbulence in the Intergalactic Medium
• Probing interstellar turbulence in spiral galaxies using HI power spectrum analysis
• Dynamics of a Supernova Envelope in a Cloudy Interstellar Medium
• Low Frequency Carbon Radio Recombination Lines I: Calculations of Departure Coefficients
• Simulations of multi-phase turbulence in jet cocoons
• Radio Synchrotron Fluctuation Statistics as a Probe of Magnetized Interstellar Turbulence
• Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds
• Supernovae feedback propagation: the role of turbulence
• 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
• Supernova-regulated ISM -- V. Space- and time-correlations
• Radiative transfer with POLARIS. II.: Modeling of synthetic Galactic synchrotron observations
• Galactic foregrounds: Spatial fluctuations and a procedure of removal
• Effects of the ISM on Detection of Low-frequency Gravitational Waves
• Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium
• Cloud formation in colliding flows: influence of the choice of cooling function
• Relationship between turbulence energy and density variance in the Solar neighbourhood molecular clouds
• Mixing matters
• Magnetic fields in star forming systems (I): Idealized synthetic signatures of dust polarization and Zeeman splitting in filaments
• When disorder looks like order: a new model to explain radial magnetic fields in young supernova remnants
• Studying Magnetohydrodynamic Turbulence with Synchrotron Polarization Dispersion
• Fundamental scales in the kinematic phase of the turbulent dynamo
• The Simons Observatory: Galactic Science Goals and Forecasts
• An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
• The clustered nature of star formation. Pre--main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud
• Evolution of Unmagnetized and Magnetized Shear Layers
• Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment: I. Formulation of the Problem and Method of Solution
• Statistical tracing of magnetic fields: comparing and improving the techniques
• The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates
• Collapse of Turbulent Cores and Reconnection Diffusion
• The Turbulent Heating Rate in Strong MHD Turbulence with Nonzero Cross Helicity
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• Plasmoid Instability in the Multiphase Interstellar Medium
• The driving of turbulence in simulations of molecular cloud formation and evolution
• Mapping Spatial Variations of HI Turbulent Properties in the Small and Large Magellanic Cloud
• Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397
• Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud II: A Parameter Study
• Faraday rotation signatures of fluctuation dynamos in young galaxies
• Correlations Between Central Massive Objects And Their Host Galaxies: From Bulgeless Spirals to Ellipticals
• Galactic magnetic fields and hierarchical galaxy formation
• Numerical code for multi-component galaxies: from N-body to chemistry and magnetic fields
• Density Power Spectrum in Turbulent Thermally Bi-stable Flows
• A semi-analytic model of the turbulent multi-phase interstellar medium
• Star formation efficiencies of molecular clouds in a galactic center environment
• The VMC Survey XXII. Hierarchical Star Formation in the 30 Doradus-N158-N159-N160 Star-Forming Complex
• Simulating Supersonic Turbulence in Magnetized Molecular Clouds
• Galactic Spiral Shocks with Thermal Instability in Vertically Stratified Galactic Disks
• Wave Decay in MHD Turbulence
• SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
• A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence
• Clustering and dynamic decoupling of dust grains in turbulent molecular clouds
• Characterizing the structure of diffuse emission in Hi-GAL maps
• The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds
• The structure and characteristic scales of molecular clouds
• Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
• Simulating Anisotropic Thermal Conduction in Supernova Remnants, Implications for the Interstellar Medium
• Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium
• Arecibo Multi-Epoch HI Absorption Measurements Against Pulsars: Tiny-Scale Atomic Structure
• Does turbulence determine the initial mass function?
• The role of initial magnetic field structure in the launching of protostellar jets
• LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
• Properties and selected implications of magnetic turbulence for interstellar medium, Local Bubble and solar wind
• Turbulent energy dissipation and intermittency in ambipolar diffusion magnetohydrodynamics
• The onset of large scale turbulence in the interstellar medium of spiral galaxies
• Galactic fountains and outflows in star forming dwarf galaxies: ISM expulsion and chemical enrichment
• Dimensional argument for the impact of turbulent support on the stellar initial mass function
• The Effect of Turbulence on Nebular Emission Line Ratios
• Nonuniversal interstellar density spectra probed by pulsars
• Mapping of the structure of the galactic magnetic field with velocity gradients: Test using star light polarization
• Measuring magnetization with rotation measures and velocity centroids in supersonic MHD turbulence
• Turbulence and particle acceleration in a relativistic plasma
• Size distribution of superbubbles
• Turbulence-induced magnetic fields in shock precursors
• Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?
• Anisotropic Turbulence in Position-Position-Velocity Space: Probing Three-Dimensional Magnetic Fields
• Hydrodynamical simulations of the decay of high-speed molecular turbulence. II. Divergence from isothermality
• Interstellar MHD Turbulence and Star Formation
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Spectral properties of magnetohydrodnamic turbulence revealed by polarization synchrotron emission with Faraday rotation
• Driven Multifluid MHD Molecular Cloud Turbulence
• Physical and chemical structure of the Serpens filament -- fast formation and gravity-driven accretion
• The driving scale -- density decorrelation scale relation in a turbulent medium
• Incidence of HI 21-cm absorption in strong FeII systems at $0.5<z<1.5$
• Cluster Formation in Contracting Molecular Clouds
• Studies of Turbulence Dissipation in Taurus Molecular Cloud with Core Velocity Dispersion (CVD)
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Density distribution function of a self-gravitating isothermal compressible turbulent fluid in the context of Molecular Clouds ensembles
• The seeds of supermassive black holes and the role of local radiation and metal spreading
• Effects of multiple-scale driving on turbulence statistics
• Testing the Turbulent Origin of the Stellar Initial Mass Function
• The link between solenoidal turbulence and slow star formation in G0.253+0.016
• The relation between the true and observed fractal dimensions of turbulent clouds
• Local support against gravity in magneto-turbulent fluids
• Can Sgr A* flares reveal the molecular gas density PDF?
• A submillimetre survey of the kinematics of the Perseus molecular cloud - III. Clump kinematics
• Study Turbulence and Probe Magnetic Field Using Gradients Technique: Application to HI-to-H2 Transition Regions
• Achieving Fast Reconnection in Resistive MHD Models via Turbulent Means
• Most of the cool CGM of star-forming galaxies is not produced by supernova feedback
• Turbulent Density Spectrum in Solar Wind Plasma
• Dense Regions in Supersonic Isothermal Turbulence
• Velocity Gradients: Magnetic Field Tomography towards the Supernova Remnant W44
• CARMA Large Area Star Formation Survey: Dense Gas in the Young L1451 Region of Perseus
• Tracing Milky Way scattering by compact extragalactic radio sources
• Low Frequency Carbon Radio Recombination Lines II: The Diffuse Interstellar Medium
• Chemical enrichment of the pre-solar cloud by supernova dust grains
• The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
• Local Molecular Gas toward the Aquila Rift Region
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• Spatial Power Spectra of Dust across the Local Group: No Constraint on Disc Scale Height
• The Nature of the Gould Belt from a Fractal Analysis of its Stellar Population
• Understanding Galaxy Outflows as the Product of Unstable Turbulent Support
• Asymmetric energy transfers in driven nonequilibrium systems and arrow of time
• Effects of Grain Alignment Efficiency on Synthetic Dust Polarization Observations of Molecular Clouds
• A global view on star formation: The GLOSTAR Galactic plane survey VIII. Formaldehyde absorption in Cygnus~X
• Centroid Velocity Statistics of Molecular Clouds
• Interstellar Polarization Survey II: General Interstellar Medium
• The Correlation Dimension of Young Stars in Dwarf Galaxies
• Fast deuterium fractionation in magnetized and turbulent filaments
• A comparison of shock-cloud and wind-cloud interactions: The longer survival of clouds in winds
• Nonlinear closures for scale separation in supersonic magnetohydrodynamic turbulence
• Topological signatures of interstellar magnetic fields - I. Betti numbers and persistence diagrams
• Methods for compressible fluid simulation on GPUs using high-order finite differences
• The Catalogue for Astrophysical Turbulence Simulations (CATS)
• Tracing Magnetic Field with Synchrotron Polarization Gradients: Parameter Study
• Tracing magnetic fields by the synergies of synchrotron emission gradients
• Searching for Molecular Outflows with Support Vector Machines: Dark Cloud Complex in Cygnus
• Mirror diffusion of cosmic rays in highly compressible turbulence near supernova remnants
• The magnetic field in the NGC 2024 FIR 5 dense core
• Insights from Simulations of Star Formation
• The structure of molecular gas associated with NGC2264: wide-field 12CO and H2 imaging
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• Nonuniversal power-law spectra in turbulent systems
• Nature of supersonic turbulence and density distribution function in the multiphase interstellar medium
• Galaxy Evolution: Modeling the Role of Non-thermal Pressure in the Interstellar medium
• Scaling properties of small-scale fluctuations in magnetohydrodynamic turbulence
• Modelling supernova driven turbulence
• Probability distribution functions of gas in M31 and M51
• The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE: Overview and first results toward DR20 from the Max Planck IRAM Observatory program (MIOP)
• The VMC Survey XXVII. Young Stellar Structures in the LMC${}^{\prime }$s Bar Star-Forming Complex
• Reconnection in weakly stochastic B-fields in 2D
• Molecular cloud formation as seen in synthetic Hi and molecular gas observations
• The role of turbulence, magnetic fields and feedback for star formation
• High-redshift Damped Ly-alpha Absorbing Galaxy Model Reproducing the N(HI)-Z Distribution
• Tidal Tails of Minor Mergers: Star Formation Efficiency in the Western Tail of NGC 2782
• Anomalous compressible mode generation by global frame projections of pure Alfven mode
• The structure and characteristic scales of the HI gas in galactic disks
• The interaction of a magnetohydrodynamical shock with a filament
• The Phase Coherence of Interstellar Density Fluctuations
• The driving mode of shock-driven turbulence
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Magnetic fields in early protostellar disk formation
• The "Maggie" filament: Physical properties of a giant atomic cloud
• Multiscale mass transport in z~6 galactic discs: fueling black holes
• Spatial variations of turbulent properties of neutral hydrogen gas in the Small Magellanic Cloud using structure function analysis
• VALES VII: Molecular and ionized gas properties in pressure balanced interstellar medium of starburst galaxies at z ~ 0.15
• A comparison of shock-cloud and wind-cloud interactions: effect of increased cloud density contrast on cloud evolution
• Hierarchical star formation in nearby galaxies
• Magnetic Field and Faraday Rotation Measure in the Turbulent Warm Ionized Medium
• Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics?
• WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
• The Late-Time Light Curves of Type Ia Supernovae: Confronting Models with Observations
• Modelling ripples in Orion with coupled dust dynamics and radiative transfer
• Modeling turbulent energy behavior and sudden viscous dissipation in compressing plasma turbulence
• Advanced Diagnostics for the Study of Linearly Polarized Emission. II: Application to Diffuse Interstellar Radio Synchrotron Emission
• Clumps as multiscale structures in cosmic noon galaxies
• Numerical viscosity and resistivity in MHD turbulence simulations
• Evidence of large scale energy cascade in the spiral galaxy NGC 5236
• Electron Distribution in the Galactic Disk - Results From a Non-Equilibrium Ionization Model of the ISM
• Accretion driven turbulence in filaments I: Non-gravitational accretion
• Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies
• Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
• Formation of OB Associations in Galaxies
• Diagnosis of 3D magnetic field and modes composition in MHD turbulence with Y-parameter
• Running with the Bulls: The frequency of star-disc encounters in the Taurus star forming region
• Observational Diagnostics for Two-Fluid Turbulence in Molecular Clouds As Suggested by Simulations
• Turbulent power distribution in the local interstellar medium
• Estimation of Magnetic Field Strength in the Turbulent Warm Ionized Medium
• Studying Anisotropy of Compressible Magnetohydrodynamic Turbulence by Synchrotron Polarization Intensity
• Magnetic fields from Multiplicative Chaos
• Irregular Magnetic Fields and the Far-Infrared Polarimetry of Dust Emission from Interstellar Clouds
• Chemo-dynamical simulations of dwarf galaxy evolution
• 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
• Probes of turbulent driving mechanisms in molecular clouds from fluctuations in synchrotron intensity
• Evolution and lifetime of transient clumps in the turbulent interstellar medium
• The structure function of Galactic \HI opacity fluctuations on AU scales based on MERLIN, VLA and VLBA data
• Orbital dynamics and extreme scattering event properties from long-term scintillation observations of PSR J1603-7202
• A kiloparsec-scale ordered magnetic field in a galaxy at z=5.6
• Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
• Multifluid magnetohydrodynamic turbulent decay
• Stability of two-fluid partially-ionised slow-mode shock fronts
• Cloud Dispersal in Turbulent Flows
• The Column Density Variance in Turbulent Interstellar Media: A Fractal Model Approach
• 3D morphology of a random field from its 2D cross-section
• The Effect of Shock Wave Duration on Star Formation and the Initial Condition of Massive Cluster Formation
• Coupling local to global star formation in spiral galaxies: the effect of differential rotation
• The Interaction Between a Pulsed Astrophysical Jet and Small-Scale Heterogeneous Media
• Simulating TeV gamma-ray morphologies of shell-type supernova remnants
• Description of turbulent dynamics in the interstellar medium: multifractal/microcanonical analysis I. Application to Herschel observations of the Musca filament
• Turbulent magneto-genesis in a collisionless plasma
• Quantifying kinematic substructure in star-forming regions with statistical tests of spatial autocorrelation
• Physics of Non-Universal Larson's Relation
• Principal Component Analysis studies of turbulence in optically thick gas
• Observations of chemical differentiation in clumpy molecular clouds
• Universal gravity-driven isothermal turbulence cascade in disk galaxies
• The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS)
• Spinning Bar and a Star-formation Inefficient Repertoire: Turbulence in Hickson Compact Group NGC7674
• Effects of grain shattering by turbulence on extinction curves in starburst galaxies
• Tearing instability in Alfvén and kinetic-Alfvén turbulence
• TIMES I: a Systematic Observation in Multiple Molecular Lines Toward the Orion A and Ophiuchus Clouds
• Massive Prestellar Cores in Radiation-magneto-turbulent Simulations of Molecular Clouds
• Hierarchical Bayesian analysis of the velocity power spectrum in supersonic turbulence
• Ionization-Gasdynamic Simulations of Wind-Blown Nebulae around Massive Stars
• A Search for correlations between turbulence and star formation in THINGS galaxies
• Star-forming regions of the Aquila rift cloud complex. II. Turbulence in molecular cores probed by NH3 emission
• On the properties of fractal cloud complexes
• The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 star-forming Clump
• Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium
• HOW-MHD: A High-Order WENO-Based Magnetohydrodynamic Code with a High-Order Constrained Transport Algorithm for Astrophysical Applications
• Gravitational Fragmentation of Extremely Metal-poor Circumstellar Discs
• Non-ideal MHD turbulent decay in molecular clouds
• A lower bound on adiabatic heating of compressed turbulence for simulation and model validation
• Structure analysis of simulated molecular clouds with the Delta-variance
• Modeling Turbulence in Galactic Centers
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• Generation of Solenoidal Modes and Magnetic Fields in Turbulence Driven by Compressive Driving
• Ram pressure stripping in elliptical galaxies: II. magnetic field effects
• Extended magnetic reconnection in kinetic plasma turbulence
• Characterization of Turbulence from Submillimeter Dust Emission
• Cloud properties across spatial scales in simulations of the interstellar medium
• Interstellar Turbulence and Star Formation
• CMB foreground measurements through broad-band radio spectro-polarimetry: prospects of the SKA-MPG telescope
• How to move ionized gas: an introduction to the dynamics of HII regions
• Kinematics of Galactic Centre clouds shaped by shear-seeded solenoidal turbulence
• The RMS Survey: Ammonia mapping of the environment of young massive stellar objects II
• Turbulence in the Harassed Galaxy NGC 4254
• Solenoidal turbulent modes and star formation efficiency in Galactic-plane molecular clouds
• R-process Rain from Binary Neutron Star Mergers in the Galactic Halo
• Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde V. The massive filament DR21
• Dust Scattering In Turbulent Media: Correlation Between The Scattered Light and Dust Column Density
• Application of Convolutional Neural Networks to Predict Magnetic Fields Directions in Turbulent Clouds
• Dust growth by accretion of molecules in supersonic interstellar turbulence
• Gravito-magnetic instabilities of Relativistic Magnetohydrodynamics
• Testing SALT Approximations with Numerical Radiation Transfer Code Part 1: Validity and Applicability
• Scaling of Turbulent Viscosity and Resistivity: Extracting a Scale-dependent Turbulent Magnetic Prandtl Number
• Dust in Clusters of Galaxies
• Turbulence in Wind-Blown Bubbles around Massive Stars
• Ram pressure stripping in elliptical galaxies: I. the impact of the interstellar medium turbulence
• FEASTS Combined with Interferometry. III. The Low Column Density HI Around M51 and Possibility of Turbulent-mixing Gas Accretion
• Density and Velocity Correlations in Isothermal Supersonic Turbulence
• The supernova-regulated ISM. IV. A comparison of simulated polarization with Planck observations
• The nature of turbulence in OMC1 at the star forming scale: observations and simulations
• When Gas Dynamics Decouples from Galactic Rotation: Characterizing ISM Circulation in Disk Galaxies
• Turbulence and Star Formation in a Sample of Spiral Galaxies
• Simulations of pre-supernova feedback in spherical clouds
• Multiline observations of hydrogen, helium, and carbon radio-recombination lines toward Orion A: A detailed dynamical study and direct determination of physical conditions
• 3D Hydrodynamic Simulations of the Galactic Supernova Remnant CTB 109
• The auto and cross angular power spectrum of the Cas A supernova remnant in radio and X-ray
• Shock identification and classification in 2D MHD compressible turbulence -- Orszag-Tang vortex
• Testing assumptions and predictions of star-formation theories
• Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
• Visibility moments and power spectrum of turbulence velocity
• Sequential Star Formation in the Young SMC Region NGC 602: Insights from ALMA
• Interactions of a shock with a molecular cloud at various stages of its evolution due to thermal instability and gravity
• Turbulent magnetic field in the HII region Sh 2-27
• The large- and small-scale CaII K structure of the Milky Way from observations of Galactic and Magellanic sightlines
• Electromagnetic thermal instability with momentum and energy exchange between electrons and ions in galaxy clusters
• On the gravitational stability of a galactic disc as a two-fluid system
• Cosmic Ray Small-Scale Anisotropies in Quasi-Linear Theory
• The Astrochemical Evolution of Turbulent Giant Molecular Clouds : I - Physical Processes and Method of Solution for Hydrodynamic, Embedded Starless Clouds
• 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
• Energy Transfer and Spectra in Simulations of Two-dimensional Compressible Turbulence
• Long-Term Evolution of Decaying MHD Turbulence in the Multiphase ISM
• Effects of the magnetic field direction on the Tsallis statistic
• The Spatial Power Spectrum and Derived Turbulent Properties of Isolated Galaxies
• CO Outflow Candidates Toward the W3/4/5 Complex II: Feedback from Candidate Outflows
• Formation of dust filaments in the diffuse envelopes of molecular clouds
• Synthetic Observations of Carbon Lines of Turbulent Flows in Diffuse Multiphase Interstellar Medium
• Turbulence evolution in MHD plasmas
• Continuum and Spectral Line Radiation from a Random Clumpy Medium
• HOPS 361-C's Jet Decelerating and Precessing Through NGC 2071 IR
• Multi log-normal density structure in Cygnus-X molecular clouds: A fitting for N-PDF without power-law
• Redshifted methanol absorption tracing infall motions of high-mass star formation regions
• Substellar fragmentation in self-gravitating fluids with a major phase transition
• CII*/CII ratio in high-redshift DLAs: ISM phase separation drives the observed bimodality of [CII] cooling rates
• Magnetic ionization-thermal instability
• Coagulation of inertial particles in supersonic turbulence
• The gas turbulence in planetary nebulae: quantification and multi-D maps from long-slit, wide-spectral range echellogram
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• Explaining the stellar initial mass function with the theory of spatial networks
• Shear, writhe and filaments: turbulence in the high latitude molecular cloud MBM 40
• Shocks in the warm neutral medium I -- Theoretical model
• Probing the Physics of Star-Formation (ProPStar) III. No evidence for dissipation of turbulence down to 20 mpc (4 000 au) scale
• 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
• Mean fields and fluctuations in compressible magnetohydrodynamic flows
• Strong turbulence and magnetic coherent structures in the interstellar medium
• The turbulence driving parameter of molecular clouds in disc galaxies
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Analytic characterization of sub-Alfvénic turbulence energetics
• The Panchromatic Hubble Andromeda Treasury. Progression of Large-Scale Star Formation across Space and Time in M31
• Star Cluster Formation in Clouds with Externally Driven Turbulence
• Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
• Gibbs Point Process Model for Young Star Clusters in M33
• Estimating statistics of sky brightness using radio interferometric observations
• Effect of turbulent velocity on the \HI intensity fluctuation power spectrum from spiral galaxies
• Finite shock model of density in supersonic turbulence
• 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
• Widespread subsonic turbulence in Ophiuchus North 1
• Formation of H2-He substellar bodies in cold conditions: Gravitational stability of binary mixtures in a phase transition
• Probing magnetic fields with Square Kilometre array and its precursors
• Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences
• Density distribution function of a self-gravitating isothermal turbulent fluid in the context of molecular clouds ensembles -- III. Virial analysis
• Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
• Spiral arm triggering of star formation
• Dust dynamics in RAMSES -- II. Equilibrium drift velocity distributions of charged dust grains
• Influence of energy exchange of electrons and ions on the long-wavelength thermal instability in magnetized astrophysical objects
• Inverse transfer of magnetic helicity in direct numerical simulations of compressible isothermal turbulence: scaling laws
• A systematic comparison of two-equation RANS turbulence models applied to shock-cloud interactions
• Does the HCN/CO ratio trace the star-forming fraction of gas? II. Variations in CO and HCN Emissivity
• Structure of iso-density sets in supersonic isothermal turbulence
• Clumpy shocks as the driver of velocity dispersion in molecular clouds: the effects of self-gravity and magnetic fields
• Shocks in the warm neutral medium II -- Origin of neutral carbon at high pressure
• Inverse transfer of magnetic helicity in direct numerical simulations of compressible isothermal turbulence: helical transfers
• Cloud structure and young star distribution in the Dragonfish complex
• HI column density statistics of the cold neutral medium from absorption studies
• Measuring the spectral index of turbulent gas with deep learning from projected density maps
• A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity
• Turbulence and galactic structure
• Simulations of the IMF in Clusters
• Role of the sonic scale in the growth of magnetic field in compressible turbulence
• Protostellar disc structure and dynamics during star formation from cloud-scale initial conditions
• The contribution of dilatational motion to energy flux in homogeneous compressible turbulence
• On the role of stochastic Fermi acceleration in setting the dissipation scale of turbulence in the interstellar medium
• Revisiting the structure function of PSR B0950+08 scintillations
• Average value of the cosmic ray injection exponent at Galactic sources
• JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium
• Prospects of Turbulence Studies in High-Energy Density Laser-Generated Plasma: Numerical Investigations in Two Dimensions
• Hydrodynamic and Magnetohydrodynamic Simulations of Wire Turbulence
• A method for detection of structure
• Uncovering neutrinos from cosmic ray factories: the Multi Point Source method
• HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
• Anisotropy in the carbon monoxide (CO) line emission across the Milky Way's disk
• The spatial distribution of stars in open clusters
• Internal Structure of Stellar Clusters: Geometry of Star Formation
• Centrally concentrated star formation in young clusters
• Cosmic Radioactivity and Galactic Chemical Evolution
• MHD turbulence-Star Formation Connection: from pc to kpc scales
• The Drag Instability in a 2D Isothermal C-shock
• The Structure of Molecular Clouds: III - A link between cloud structure and star formation mode
• Turbulence in the Molecular Interstellar Medium
• Revealing the drag instability in one-fluid nonideal MHD simulations of a 1D isothermal C-shock
• Why most molecular clouds are gravitationally dominated
• On the interaction of a thin, supersonic shell with a molecular cloud
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Density PDFs of diffuse gas in the Milky Way
• Shock fragmentation model for gravitational collapse
• Supernova origin of galactic turbulence revealed by superbubbles
• Recent Developments on the HI Gas of Low-Redshift Galaxies Seen by the 21cm Emission Lines
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
• CO Structures with Narrow Lines in Nearby Quiescent Regions
• From 2D to 3D: Recovering Turbulent Density Dispersions from Noisy Data
• High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields
• Hypersonic Molecular Shocks in Star Forming Regions
• What does it mean to take the mean? The effect of the averaging scale on the characterization of interstellar turbulence
• Direct power spectral density estimation from structure functions without Fourier transforms
• Heavy interstellar scattering toward the near end of the Galactic bar
• Acceleration of Energetic Particles through Reconnection of Weakly Stochastic Magnetic Field
• Loose threads: parsec-scale filamentation in the high Galactic latitude molecular clouds MBM 3 and MBM 16
• Intermittency and non-universality of pair dispersion in isothermal compressible turbulence
• Advection by Compressible Turbulent Flows: Renormalization Group Study of Vector and Tracer Admixture
• The interdependence between density PDF, CMF and IMF and their relation with Mach number in simulations
• Turbulence induced additional deceleration in relativistic shock wave propagation: implications for gamma-ray burst
• Thermal instability and multiphase dynamics in the ISM with polybaric pressure effects
• Interstellar scattering - New diagnostics of pulsars and the ISM
• Dynamical Evolution of a Supernova Driven Turbulent Interstellar Medium
• The signature of large scale turbulence driving on the structure of the interstellar medium
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies
• Supernovae and photoionizing feedback in spiral arm molecular clouds
• Correlations of gas, dust and young stellar populations in the spiral galaxy NGC 7331