Dissipation in Compressible MHD Turbulence

Abstract

We report results of a three dimensional, high resolution (up to 512^3) numerical investigation of supersonic compressible magnetohydrodynamic turbulence. We consider both forced and decaying turbulence. The model parameters are appropriate to conditions found in Galactic molecular clouds. We find that the dissipation time of turbulence is of order the flow crossing time or smaller, even in the presence of strong magnetic fields. About half the dissipation occurs in shocks. Weak magnetic fields are amplified and tangled by the turbulence, while strong fields remain well ordered.

5 pages, 3 Postscript figures, LaTeX, accepted by Ap.J.Lett

References in corpus (1)

• Kinetic Energy Decay Rates of Supersonic and Super-Alfvenic Turbulence in Star-Forming Clouds

Cited by in corpus (379)

• Star Formation in the Milky Way and Nearby Galaxies
• Theory of Star Formation
• Control of star formation by supersonic turbulence
• Toward Understanding Massive Star Formation
• Interstellar Turbulence I: Observations and Processes
• The Neutral Atomic Phases of the ISM in the Galaxy
• A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs
• The Stellar IMF from Turbulent Fragmentation
• The Formation of Massive Stars from Turbulent Cores
• Cold Dark Clouds: The Initial Conditions for Star Formation
• Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
• Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
• Radiation Pressure Supported Starburst Disks and AGN Fueling
• The Formation of a Star Cluster: Predicting the Properties of Stars and Brown Dwarfs
• The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
• Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
• Compressible Magnetohydrodynamic Turbulence: mode coupling, scaling relations, anisotropy, new regime and astrophysical implications
• Star Formation in a Crossing Time
• The Resolved Properties of Extragalactic Giant Molecular Clouds
• The Energy Dissipation Rate of Supersonic, Magnetohydrodynamic Turbulence in 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
• Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
• A Super-Alfvenic Model of Dark Clouds
• Massive Stars: Their Environment and Formation
• Secular Evolution in Disk Galaxies
• The Physics of Star Formation
• Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
• What is Driving the HI Velocity Dispersion?
• Star Formation from Galaxies to Globules
• A Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport
• On the Role of Massive Stars in the Support and Destruction of Giant Molecular Clouds
• The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function
• Simulating the formation of molecular clouds. I. Slow formation by gravitational collapse from static initial conditions
• The Formation of Close Binary Systems by Dynamical Interactions and Orbital Decay
• One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-Gravitating Media
• Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
• Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
• Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts
• The Formation of Stellar Clusters: Gaussian Cloud Conditions I
• The Turbulent Shock Origin of Proto--Stellar Cores
• The Formation of Low-Mass Binary Star Systems Via Turbulent Fragmentation
• The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation
• Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology
• Protostellar Turbulence Driven by Collimated Outflows
• Modeling UV Radiation Feedback from Massive Stars: II. Dispersal of Star-Forming Giant Molecular Clouds by Photoionization and Radiation Pressure
• Molecular cloud evolution. I. Molecular cloud and thin CNM sheet formation
• The Interaction of High-Speed Turbulence with Flames: Global Properties and Internal Flame Structure
• Flows, Fragmentation, and Star Formation. I. Low-mass Stars in Taurus
• Equilibrium Star Cluster Formation
• Relativistic jet feedback in high-redshift galaxies I: Dynamics
• Molecular Evolution in Collapsing Prestellar Cores III: Contraction of A Bonnor-Ebert Sphere
• The Fractal Density Structure in Supersonic Isothermal Turbulence: Solenoidal versus Compressive Energy Injection
• On the Rapid Collapse and Evolution of Molecular Clouds
• Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
• Kinetic and Structural Evolution of Self-gravitating, Magnetized Clouds: 2.5-Dimensional Simulations of Decaying Turbulence
• The CI lines as tracers of molecular gas, and their prospects at high redshifts
• Molecular Cloud Formation Behind Shock Waves
• The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016
• Feedback-regulated star formation in molecular clouds and galactic discs
• Three Dimensional Hydrodynamic Simulations of Multiphase Galactic Disks with Star Formation Feedback: I. Regulation of Star Formation Rates
• Cluster Formation in Protostellar Outflow-Driven Turbulence
• On the universality of interstellar filaments: theory meets simulations and observations
• The Global Evolution of Giant Molecular Clouds. I: Model Formulation and Quasi-Equilibrium Behavior
• Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
• Partially Ionized Plasmas in Astrophysics
• The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim 2.6$ to $z\sim 0.6$ with KMOS${}^{3D}$
• Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model
• The effect of magnetic fields on star cluster formation
• Theoretical Models of Polarized Dust Emission from Protostellar Cores
• The Lifetimes and Evolution of Molecular Cloud Cores
• Gravity-driven Turbulence in Galactic Disks
• Challenges in Planet Formation
• Protostellar Disks: Formation, Fragmentation, and the Brown Dwarf Desert
• On the Structure of the Orion A Cloud and the Formation of the Orion Nebula Cluster
• The Interaction of High-Speed Turbulence with Flames: Turbulent Flame Speed
• The Formation of Stellar Clusters: Gaussian Initial Conditions II
• New OH Zeeman measurements of magnetic field strengths in molecular clouds
• Turbulent Driving Scales in Molecular Clouds
• Magnetic field amplification in turbulent astrophysical plasmas
• A Model for the Origin of Bursty Star Formation in Galaxies
• Comments on Inferences of Star Formation Histories and Birthlines
• Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies
• Kinetic turbulence in relativistic plasma: from thermal bath to non-thermal continuum
• A Dynamical Model for the Formation of Gas Rings and Episodic Starbursts Near Galactic Centres
• Observational Constraints on the Ages of Molecular Clouds and the Star-Formation Timescale: Ambipolar-Diffusion--Controlled or Turbulence-Induced Star Formation?
• Scaling relations of supersonic turbulence in star-forming molecular clouds
• Ionizing feedback from massive stars in massive clusters III: Disruption of partially unbound clouds
• SILCC-Zoom: The dynamical and chemical evolution of molecular clouds
• The Link between Magnetic Fields and Filamentary Clouds: Bimodal Cloud Orientations in the Gould Belt
• Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
• Simulating star formation in molecular cores II. The effects of different levels of turbulence
• On the Dynamics and Evolution of Gravitational Instability-Dominated Disks
• Self-similar Fragmentation Regulated by Magnetic Fields in a Massive Star Forming Filament
• The Global Evolution of Giant Molecular Clouds II: The Role of Accretion
• Growth of Magnetic Fields Induced by Turbulent Motions
• The Physics of Star Cluster Formation and Evolution
• Evolving Gravitationally Unstable Disks Over Cosmic Time: Implications For Thick Disk Formation
• Quiescent Cores and the Efficiency of Turbulence-Accelerated, Magnetically Regulated Star Formation
• The molecular cloud lifecycle
• The impact of turbulence and magnetic field orientation on star forming filaments
• Strong Anisotropic MHD Turbulence with Cross Helicity
• Accretion-Driven Turbulence and the Transition to Global Instability in Young Galaxy Disks
• Analysis of Clumps in Molecular Cloud Models: Mass Spectrum, Shapes, Alignment and Rotation
• Turbulence, Magnetic Reconnection in Turbulent Fluids and Energetic Particle Acceleration
• The Generation and Dissipation of Interstellar Turbulence - Results from Large Scale High Resolution Simulations
• Organic Molecules in the Galactic Center. Hot Core Chemistry without Hot Cores
• On the properties of young multiple stars
• 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 Magnetohydrodynamic Kelvin-Helmholtz Instability: A Three-Dimensional Study of Nonlinear Evolution
• Gravitational Instabilities in Two-Component Galaxy Disks with Gas Dissipation
• Scaling Relations of Star-Forming Regions: from kpc-size clumps to HII regions
• Transition of the initial mass function in the metal-poor environments
• The Formation of the First Stars in the Universe
• On the Thermonuclear Runaway in Type Ia Supernovae: How to run away?
• The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disk turbulence in z~0.9 star-forming galaxies
• Adiabatic Heating of Contracting Turbulent Fluids
• Non-universal star formation efficiency in turbulent ISM
• The Field Condition: A New Constraint of Spatial Resolution in Simulations of the nonlinear Development of Thermal Instability
• Spectral Properties of Compressible Magnetohydrodynamic Turbulence from Numerical Simulations
• Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
• Star formation in unbound giant molecular clouds: the origin of OB associations?
• Ram-pressure stripped molecular gas in the Virgo spiral galaxy NGC 4522
• Steady Outflows in Giant Clumps of High-z Disk Galaxies During Migration and Growth by Accretion
• Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies
• Supernova feedback in a local vertically stratified medium: interstellar turbulence and galactic winds
• A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces: I. Cloud-scale Gas Motions
• Algorithmic comparisons of decaying, isothermal, supersonic turbulence
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Reprocessed Radiation Feedback from Nascent Super Star Clusters
• Survival of Star-Forming Giant Clumps in High-Redshift Galaxies
• The Spectral Correlation Function -- A New Tool for Analyzing Spectral-Line Maps
• Protostellar outflow-driven turbulence
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• Density Probability Distribution Functions in Supersonic Hydrodynamic and MHD Turbulence
• Comparison of spectral slopes of magnetohydrodynamic and hydrodynamic turbulence and measurements of alignment effects
• Incorporating the molecular gas phase in galaxy-size numerical simulations: first applications in dwarf galaxies
• Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds
• Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• Effects of Magnetic Field Strength and Orientation on Molecular Cloud Formation
• Gravitational Collapse and Filament Formation: Comparison with the Pipe Nebula
• A model for the formation of stellar associations and clusters from giant molecular clouds
• High resolution 21 cm mapping of the Ursa Major Galactic cirrus: power spectra of the high-latitude HI gas
• Modeling a high mass turn down in the stellar initial mass function
• The Deuterium Fractionation Timescale in Dense Cloud Cores: A Parameter Space Exploration
• The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
• Star Formation in Space and Time: The Orion Nebula Cluster
• Adaptive Mesh Fluid Simulations on GPU
• A turbulent MHD model for molecular clouds and a new method of accretion on to star-forming cores
• Cold Milky Way Hi gas in filaments
• Physical Processes in Star Formation
• Pressure Relations and Vertical Equilibrium in the Turbulent, Multiphase ISM
• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• Magnetically Regulated Star Formation in Turbulent Clouds
• Centrally condensed turbulent cores: Massive stars or fragmentation?
• Outflow Driven Turbulence in Molecular Clouds
• The Temperature of Interstellar Clouds from Turbulent Heating
• The Nature of the Velocity Field in Molecular Clouds. I. The Non-Magnetic Case
• The Effects of Magnetic Fields and Protostellar Feedback on Low-mass Cluster Formation
• Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons
• Building Giant-Planet Cores at a Planet Trap
• Damping of Alfven waves by Turbulence and its Consequences: from Cosmic-Rays Streaming to Launching Winds
• The dependence of the sub-stellar IMF on the initial conditions for star formation
• Mixing in Supersonic Turbulence
• Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
• Turbulence and cooling in galaxy cluster cores
• Structure of Stationary Strong Imbalanced Turbulence
• Can Protostellar Jets Drive Supersonic Turbulence in Molecular Clouds?
• Protostellar mass accretion rates from gravoturbulent fragmentation
• Formation and loss of hierarchical structure in two-dimensional MHD simulations of wave-driven turbulence in interstellar clouds
• Structure and Stability of Phase Transition Layers in the Interstellar Medium
• Extending the Shakura-Sunyaev approach to a strongly magnetized accretion disc model
• Molecular line mapping of the giant molecular cloud associated with RCW 106 - II. Column density and dynamical state of the clumps
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: I. Turbulence Statistics
• On the effect of cosmological inflow on turbulence and instability in galactic discs
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• Modeling The Molecular Composition in an AGN Disk
• Modeling protoplanetary disk SEDs with artificial neural networks: Revisiting the viscous disk model and updated disk masses
• The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds
• Molecular Outflows From the Protocluster, Serpens South
• Observing Simulated Protostars with Outflows: How Accurate are Protostellar Properties Inferred from SEDs?
• Bondi-Hoyle-Littleton accretion and the upper mass stellar IMF
• Warm Molecular Gas Traced with CO J=7->6 in the Galaxy's Central 2 Parsecs: Dynamical Heating of the Circumnuclear Disk
• Core Mass Function: The Role of Gravity
• Modeling UV Radiation Feedback from Massive Stars: I. Implementation of Adaptive Ray Tracing Method and Tests
• Gas Properties and Implications for Galactic Star Formation in Numerical Models of the Turbulent, Multiphase ISM
• Role of Cosmic Ray Streaming and Turbulent Damping in Driving Galactic Winds
• A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies
• On the Appearance of Thresholds in the Dynamical Model of Star Formation
• Protostellar Angular Momentum Evolution during Gravoturbulent Fragmentation
• Physical Properties of Dense Cores in the Rho Ophiuchi Main Cloud and A Significant Role of External Pressures in Clustered Star Formation
• The first million years of the Sun: A calculation of formation and early evolution of a solar-mass star
• Star-Gas Surface Density Correlations in Twelve Nearby Molecular Clouds I: Data Collection and Star-Sampled Analysis
• The structure of self-gravitating clouds
• Star Formation in Transient Molecular Clouds
• Scale-free gravitational collapse as the origin of $\rho \sim r^{-2}$ density profile -- a possible role of turbulence in regulating gravitational collapse
• Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud
• Interstellar Turbulence Driving by Galactic Spiral Shocks
• Diffusion in supersonic, turbulent, compressible flows
• Ambipolar Drift Heating in Turbulent Molecular Clouds
• Forced turbulence in thermally bistable gas: A parameter study
• Damping of MHD turbulence in Solar Flares
• Is molecular cloud turbulence driven by external supernova explosions?
• Are fibres in molecular cloud filaments real objects?
• Impact of Winds from Intermediate-Mass Stars on Molecular Cloud Structure and Turbulence
• Turbulent dissipation in the ISM: the coexistence of forced and decaying regimes and implications for galaxy formation and evolution
• A Case Study of Low-Mass Star Formation
• Shock Waves and Energy Dissipation in Magnetohydrodynamic Turbulence
• Formation of the Hub-Filament System G33.92+0.11: Local Interplay between Gravity, Velocity, and Magnetic Field
• HI Power Spectra and the Turbulent ISM of Dwarf Irregular Galaxies
• Evolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters. I. The Effect of Injection Energy and Redshift
• Magnetic fields in the massive dense cores of DR21 filament: weakly magnetized cores in a strongly magnetized filament
• Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. I. 60Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous ISM
• The Formation of Stellar Clusters: Time Varying Protostellar Accretion Rates
• The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback
• An Explicit Scheme for Incorporating Ambipolar Diffusion in a Magnetohydrodynamics Code
• Energy dynamics and current sheet structure in fluid and kinetic simulations of decaying magnetohydrodynamic turbulence
• Signatures of star cluster formation by cold collapse
• Molecular Tracers of Turbulent Shocks in Giant Molecular Clouds
• Parsec-Scale Herbig-Haro Outflows from Intermediate Mass Stars
• MODEST-1: Integrating Stellar Evolution and Stellar Dynamics
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• The SAMI Galaxy Survey: Gas velocity dispersions in low-$z$ star-forming galaxies and the drivers of turbulence
• Enhanced Core Formation Rate in a Turbulent Cloud by Self-gravity
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• The Great PV Ceph Outflow: A Case Study in Outflow-Cloud Interaction
• ALMA observations of NGC 6334S $-$ I: Forming massive stars and cluster in subsonic and transonic filamentary clouds
• High-order Magnetohydrodynamics for Astrophysics with an Adaptive Mesh Refinement Discontinuous Galerkin Scheme
• Protostellar Outflow Evolution in Turbulent Environments
• Turbulent magnetic relaxation in pulsar wind nebulae
• Simulating Supersonic Turbulence in Galaxy Outflows
• Can magnetized turbulence set the mass scale of stars?
• Local Turbulence Simulations for the Multiphase ISM
• Statistics of Core Lifetimes in Numerical Simulations of Turbulent, Magnetically Supercritical Molecular Clouds
• Hydrodynamical simulations of the decay of high-speed molecular turbulence. I. Dense molecular regions
• What drives the velocity dispersion of ionized gas in star-forming galaxies?
• Technique for separating velocity and density contributions in spectroscopic data and its application to studying turbulence and magnetic fields
• Modest-2: A Summary
• Turbulence Dynamo in Galaxy Clusters
• Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies
• Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
• Reconnection-controlled decay of magnetohydrodynamic turbulence and the role of invariants
• Magnetized converging flows towards the hot core in the intermediate/high-mass star-forming region NGC 6334 V
• Statistical analysis of the interplay between magnetic fields and filaments hosting Planck Galactic Cold Clumps
• Interstellar Phase Transitions Stimulated by Time-dependent Heating
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• The Density Distribution in Turbulent Bi-stable Flows
• Dynamical Expansion of H II Regions from Ultracompact to Compact Sizes in Turbulent, Self-Gravitating Molecular Clouds
• Linewidth Differences of Neutrals and Ions Induced by MHD Turbulence
• On the turbulence driving mode of expanding HII regions
• On the compressive nature of turbulence driven by ionising feedback in the pillars of the Carina Nebula
• The Origin of Exponential Star-forming Disks
• The Turbulent Interstellar Medium
• MHD Turbulence, Turbulent Dynamo and Applications
• Particle energization in relativistic plasma turbulence: solenoidal versus compressive driving
• On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions
• Protostellar Jets and Turbulence in Molecular Clouds: The Role of Interactions
• The interstellar medium distribution, gas kinematics, and system dynamics of the far-infrared luminous quasar SDSS J2310+1855 at $z=6.0$
• Studying Magnetohydrodynamic Turbulence with Synchrotron Polarization Dispersion
• Numerical simulations of supernova remnants in turbulent molecular clouds
• Gas Accretion Can Drive Turbulence in Galaxies
• Infall models of Class 0 protostars
• Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud II: A Parameter Study
• A scaling relation for the molecular cloud lifetime in Milky Way-like galaxies
• The driving of turbulence in simulations of molecular cloud formation and evolution
• The physical drivers of gas turbulence in simulated disc galaxies
• Ambipolar Diffusion Heating in Turbulent Systems
• Scale-free Equilibria of Magnetized Polytropic Clouds
• SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
• The MHD Kelvin-Helmholtz Instability III: The Role of Sheared Magnetic Field in Planar Flows
• A Prescription for Star Formation Feedback: The Importance of Multiple Shell Interactions
• Mid-J CO observations of Perseus B1-East 5: evidence for turbulent dissipation via low-velocity shocks
• The CH+ Abundance in Turbulent, Diffuse Molecular Clouds
• Accretion driven turbulence in filaments II: Effects of self-gravity
• Predicting HCN, HCO+, multi-transition CO, and dust emission of star-forming galaxies From local spiral and ultraluminous infrared galaxies to high-z star-forming and submillimeter galaxies
• The role of the turbulence driving mode for the Initial Mass Function
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Interstellar MHD Turbulence and Star Formation
• Testing the Turbulent Origin of the Stellar Initial Mass Function
• Expanding CO Shells in the Orion A Molecular Cloud
• Star Cluster Formation from Turbulent Clumps. II. Gradual Star Cluster Formation
• The seeds of supermassive black holes and the role of local radiation and metal spreading
• The Interstellar Medium and Star Formation of Galactic Disks. I. ISM and GMC properties with Diffuse FUV and Cosmic Ray Backgrounds
• A New Method for Constraining Molecular Cloud Thickness: A study of Taurus, Perseus and Ophiuchus
• The link between solenoidal turbulence and slow star formation in G0.253+0.016
• Can Sgr A* flares reveal the molecular gas density PDF?
• Turbulent Density Spectrum in Solar Wind Plasma
• Signatures of fast and slow magnetohydrodynamic shocks in turbulent molecular clouds
• Impact of Cosmic-Ray Feedback on Accretion and Chemistry in Circumstellar Disks
• Anisotropic cosmic-ray diffusion in isotropic Kolmogorov turbulence
• How astrophysical mean field dynamos can circumvent existing quenching constraints
• GMC Collisions as Triggers of Star Formation. VI. Collision-Induced Turbulence
• A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
• Dense Regions in Supersonic Isothermal Turbulence
• A new method for measuring the 3D turbulent velocity dispersion of molecular clouds
• Multiple Radial Cool Molecular Filaments in NGC 1275
• The effects of ionization feedback on star formation: A case study of the M16 H II region
• Insights from Simulations of Star Formation
• Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action
• Compression of turbulent magnetized gas in Giant Molecular Clouds
• Evidence for Decay of Turbulence by MHD Shocks in Molecular Clouds via CO Emission
• Constraints on Stirring and Dissipation of MHD Turbulence in Molecular Clouds
• As a matter of force - Systematic biases in idealized turbulence simulations
• An Exploration of the Statistical Signatures of Stellar Feedback
• Magnetic Field and Faraday Rotation Measure in the Turbulent Warm Ionized Medium
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds III: SLED fitting
• Irregular Magnetic Fields in Interstellar Clouds and the Linear Polarization of Starlight
• Interaction of the magnetorotational instability with hydrodynamic turbulence in accretion disks
• Irregular Magnetic Fields and the Far-Infrared Polarimetry of Dust Emission from Interstellar Clouds
• Formation of OB Associations in Galaxies
• Estimation of Magnetic Field Strength in the Turbulent Warm Ionized Medium
• Wind-Driven Gas Networks and Star Formation in Galaxies: Reaction-Advection Hydrodynamic Simulations
• Wide binary stars formed in the turbulent interstellar medium
• Long-lived Magnetic-Tension-Driven Modes in a Molecular Cloud
• The Energetics of Molecular Gas in NGC 891 from H2 and FIR Spectroscopy
• Accretion driven turbulence in filaments I: Non-gravitational accretion
• Spectral characterisation of inertial particle clustering in turbulence
• Velocity Anisotropy in Self-Gravitating Molecular Clouds. I: Simulation
• On the Effects of Dissipative Turbulence on the Narrow Emission-Line Ratios in Seyfert Galaxies
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds I
• Effects of turbulence in the Circumnuclear Disk
• Toward Understanding the Origin of Turbulence in Molecular Clouds: Small Scale Structures as Units of Dynamical Multi-Phase Interstellar Medium
• Scaling, Intermittency and Decay of MHD Turbulence
• Supersonic turbulence in 3D isothermal flow collision
• Turbulence decay and cloud core relaxation in molecular clouds
• Physics of Non-Universal Larson's Relation
• Description of turbulent dynamics in the interstellar medium: multifractal/microcanonical analysis I. Application to Herschel observations of the Musca filament
• Anisotropy of Magnetohydrodynamic Turbulence and the Polarized Spectra of OH Masers
• Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence
• Identification of a Fundamental Transition in a Turbulently-Supported Interstellar Medium
• Probing the nature of dissipation in compressible MHD turbulence
• A review of the theory of incompressible MHD turbulence
• Cloud properties across spatial scales in simulations of the interstellar medium
• Modeling Turbulence in Galactic Centers
• Molecular Clouds: Internal Properties, Turbulence, Star Formation and Feedback
• Irregular Magnetic Fields in Interstellar Clouds and Variations in the Observed Circular Polarization of Spectral Lines
• Basic Properties of Compressible MHD Turbulence: Implications for Molecular Clouds
• Twofold effect of Alfven waves on the transverse gravitational instability
• X-raying molecular clouds with a short flare: probing statistics of gas density and velocity fields
• Structure of dynamical condensation fronts in the interstellar medium
• The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
• MaLeFiSenta: Machine Learning for FilamentS Identification and orientation in the ISM
• Observations and Theory of Star Cluster Formation
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Long-Term Evolution of Decaying MHD Turbulence in the Multiphase ISM
• Nonlinear Criterion for the Stability of Molecular Clouds
• Spectroscopic infrared extinction mapping as a probe of grain growth in IRDCs
• Turbulent Fragmentation and Star Formation
• On turbulent fragmentation and the origin of the stellar IMF
• HOPS 361-C's Jet Decelerating and Precessing Through NGC 2071 IR
• Compressible MHD Turbulence: Implications for Molecular Cloud and Star Formation
• Molecular Line Profiles from a Core Forming in a Turbulent Cloud
• Fragmentation and Structure Formation
• Protostellar Outflows: a window to the past
• From 10 Kelvin to 10 TeraKelvin: Insights on the Interaction Between Cosmic Rays and Gas in Starbursts
• Planet formation: key mechanisms and global models
• Shocks in the warm neutral medium I -- Theoretical model
• Tracing the magnetic field morphology of the LDN 1172/1174 cloud complex
• Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Length-scales and Dynamics of Carina's Western Wall
• Dancing with the stars: Stirring up extraordinary turbulence in Galactic center clouds
• Galactic Traversability: A New Concept for Extragalactic SETI
• From Gas to Stars over Cosmic Time
• Turbulence and galactic structure
• A feedback compression star formation model and the black hole - bulge relations
• Historical perspective on astrophysical MHD simulations
• Which Molecular Cloud Structures Are Bound?
• The Drag Instability in a 2D Isothermal C-shock
• Turbulent Action at a Distance due to Stellar Feedback in Magnetized Clouds
• High Mass Star Formation by Gravitational Collapse of Massive Cores
• Star Formation from Turbulent Fragmentation
• Magnetic field of a ring-like shape molecular cloud
• Turbulence, Feedback, and Slow Star Formation
• Why most molecular clouds are gravitationally dominated
• From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs -- Modelling the molecular emission of a parsec-scale torus as found in NGC1068
• Supernova origin of galactic turbulence revealed by superbubbles