Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models

Abstract

We use 3D numerical MHD simulations to follow the evolution of cold, turbulent, gaseous systems with parameters representing GMC conditions. We study three cloud simulations with varying mean magnetic fields, but identical initial velocity fields. We show that turbulent energy is reduced by a factor two after 0.4-0.8 flow crossing times (2-4 Myr), and that the magnetically supercritical cloud models collapse after ~6 Myr, while the subcritical cloud does not collapse. We compare density, velocity, and magnetic field structure in three sets of snapshots with matched Mach numbers. The volume and column densities are both log-normally distributed, with mean volume density a factor 3-6 times the unperturbed value, but mean column density only a factor 1.1-1.4 times the unperturbed value. We use a binning algorithm to investigate the dependence of kinetic quantities on spatial scale for regions of column density contrast (ROCs). The average velocity dispersion for the ROCs is only weakly correlated with scale, similar to the mean size-linewidth relation for clumps within GMCs. ROCs are often superpositions of spatially unconnected regions that cannot easily be separated using velocity information; the same difficulty may affect observed GMC clumps. We analyze magnetic field structure, and show that in the high density regime, total magnetic field strengths increase with density with logarithmic slope 1/3 -2/3. Mean line-of-sight magnetic field strengths vary widely across a projected cloud, and do not correlate with column density. We compute simulated interstellar polarization maps at varying orientations, and determine that the Chandrasekhar-Fermi formula multiplied by a factor ~0.5 yields a good estimate of the plane-of sky magnetic field strength provided the dispersion in polarization angles is < 25 degrees.

56 pages, 25 figures; Ap.J., accepted

References in corpus (3)

• Star Formation in a Crossing Time
• Formation and loss of hierarchical structure in two-dimensional MHD simulations of wave-driven turbulence in interstellar clouds
• On the Effects of Projection on Morphology

Cited by in corpus (593)

• Theory of Star Formation
• Control of star formation by supersonic turbulence
• Interstellar Turbulence I: Observations and Processes
• The Stellar IMF from Turbulent Fragmentation
• Cold Dark Clouds: The Initial Conditions for Star Formation
• Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
• 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
• The Dark Molecular Gas
• Analytical theory for the initial mass function: CO clumps and prestellar cores
• Structural Analysis of Molecular Clouds: Dendrograms
• Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
• Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation
• Towards a complete accounting of energy and momentum from stellar feedback in galaxy formation simulations
• Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
• The Disruption of Giant Molecular Clouds by Radiation Pressure and the Efficiency of Star Formation in Galaxies
• The Star Formation Rate of Supersonic MHD Turbulence
• Probing the evolution of molecular cloud structure: From quiescence to birth
• Stellar, Brown Dwarf, and Multiple Star Properties from Hydrodynamical Simulations of Star Cluster Formation
• The hierarchical formation of a stellar cluster
• Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
• Massive star formation: Nurture, not nature
• The Formation Mechanism of Brown Dwarfs
• Magnetic Fields in the Formation of Sun-Like Stars
• Physical properties of molecular clouds for the entire Milky Way disk
• Star Formation Efficiencies and Lifetimes of Giant Molecular Clouds in the Milky Way
• A General Model for the CO-H2 Conversion Factor in Galaxies with Applications to the Star Formation Law
• The Physics of Star Formation
• Numerical Tests of Fast Reconnection in Weakly Stochastic Magnetic Fields
• Turbulent molecular clouds
• What is Driving the HI Velocity Dispersion?
• On the diversity and statistical properties of protostellar discs
• Formation of globular clusters in hierarchical cosmology
• Star Formation from Galaxies to Globules
• On the Role of Massive Stars in the Support and Destruction of Giant Molecular Clouds
• The Formation of Close Binary Systems by Dynamical Interactions and Orbital Decay
• The Structure of the Interstellar Medium of Star Forming Galaxies
• Dispersion of Magnetic Fields in Molecular Clouds. I
• The Turbulent Shock Origin of Proto--Stellar Cores
• The Importance of Radiative Feedback for the Stellar Initial Mass Function
• Star Formation Properties of a Large Sample of Irregular Galaxies
• The COMPLETE Survey of Star-Forming Regions: Phase I Data
• The relation between gas and dust in the Taurus Molecular Cloud
• An Imprint of Molecular Cloud Magnetization in the Morphology of the Dust Polarized Emission
• Density Fluctuations in MHD Turbulence: Spectra, Intermittency and Topology
• Protostellar Turbulence Driven by Collimated Outflows
• Modeling Molecular Hydrogen and Star Formation in Cosmological Simulations
• The PdBI Arcsecond Whirlpool Survey (PAWS). I. A Cloud-Scale/Multi-Wavelength View of the Interstellar Medium in a Grand-Design Spiral Galaxy
• SCUBA Polarization Measurements of the Magnetic Field Strengths in the L183, L1544, and L43 Prestellar Cores
• The propagation of uncertainties in stellar population synthesis modeling II: The challenge of comparing galaxy evolution models to observations
• Dispersion of Magnetic Fields in Molecular Clouds. II
• How stellar feedback simultaneously regulates star formation and drives outflows
• 2MASS wide field extinction maps - I. The Pipe nebula
• Flows, Fragmentation, and Star Formation. I. Low-mass Stars in Taurus
• The initial conditions of isolated star formation - VI. SCUBA mapping of prestellar cores
• The Fractal Density Structure in Supersonic Isothermal Turbulence: Solenoidal versus Compressive Energy Injection
• On the interplay between star formation and feedback in galaxy formation simulations
• Magnetic Fields in High-Mass Infrared Dark Clouds
• Molecular Cloud Formation Behind Shock Waves
• The "True" Column Density Distribution in Star-Forming Molecular Clouds
• Magnetic Fields and Massive Star Formation
• Studies of regular and random magnetic fields in the ISM: statistics of polarization vectors and the Chandrasekhar-Fermi technique
• Feedback-regulated star formation in molecular clouds and galactic discs
• Density Studies of MHD Interstellar Turbulence: Statistical Moments, Correlations and Bispectrum
• Magnetically Regulated Star Formation in 3D: The Case of Taurus Molecular Cloud Complex
• The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State
• Effects of the Equation of State on the Formation of Star Clusters
• On the [CII]-SFR relation in high redshift galaxies
• Modeling CO Emission: I. CO as a Column Density Tracer and the X-Factor in Molecular Clouds
• WFCAM, Spitzer-IRAC and SCUBA observations of the massive star forming region DR21/W75: I. The collimated molecular jets
• Physical vs. Observational Properties of Clouds in Turbulent Molecular Cloud Models
• Magnetic Field Diagnostics Based on Far-Infrared Polarimetry: Tests Using Numerical Simulations
• Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
• Partially Ionized Plasmas in Astrophysics
• Analytical theory for the initial mass function: II. Properties of the flow
• A robust numerical scheme for highly compressible magnetohydrodynamics: Nonlinear stability, implementation and tests
• A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
• The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt
• Modelling CO formation in the turbulent interstellar medium
• Theoretical Models of Polarized Dust Emission from Protostellar Cores
• Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
• The Lifetimes and Evolution of Molecular Cloud Cores
• The CO-H2 Conversion Factor in Disc Galaxies and Mergers
• Gravity-driven Turbulence in Galactic Disks
• The Magnetic Field in Taurus Probed by Infrared Polarization
• Radiation-magnetohydrodynamic simulations of HII regions and their associated PDRs in turbulent molecular clouds
• A General Theory of Turbulent Fragmentation
• High-dynamic-range extinction mapping of infrared dark clouds: Dependence of density variance with sonic Mach number in molecular clouds
• Turbulent Driving Scales in Molecular Clouds
• Comments on Inferences of Star Formation Histories and Birthlines
• Kolmogorov-Burgers Model for Star Forming Turbulence
• Quiescent and coherent cores from gravoturbulent fragmentation
• The JCMT BISTRO Survey: The magnetic field strength in the Orion A filament
• The Two States of Star Forming Clouds
• On the evolution of a star cluster and its multiple stellar systems following gas dispersal
• A Dynamical Model for the Formation of Gas Rings and Episodic Starbursts Near Galactic Centres
• High- and Low-Mass Star Forming Regions from Hierarchical Gravitational Fragmentation. High local Star Formation Rates with Low Global Efficiencies
• 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
• Characterizing Magnetohydrodynamic Turbulence in the Small Magellanic Cloud
• Magnetically Aligned Velocity Anisotropy in the Taurus Molecular Cloud
• Density structure of the interstellar medium and the star formation rate in galactic disks
• A Theory for the Excitation of CO in Star Forming Galaxies
• Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: II. Control of the \HII Region Parameters
• First results from BISTRO -- a SCUBA-2 polarimeter survey of the Gould Belt
• The Link between Magnetic Fields and Filamentary Clouds: Bimodal Cloud Orientations in the Gould Belt
• Three-Dimensional Simulations of Parker, Magneto-Jeans, and Swing Instabilities in Shearing Galactic Gas Disks
• Self-similar Fragmentation Regulated by Magnetic Fields in a Massive Star Forming Filament
• The Turbulent Warm Ionized Medium: Emission Measure Distribution and MHD Simulations
• A Fractal Origin for the Mass Spectrum of Interstellar Clouds: II. Cloud Models and Power Law Slopes
• Star Cluster Formation in Turbulent, Magnetized Dense Clumps with Radiative and Outflow Feedback
• The Probability Distribution Function of Column Density in Molecular Clouds
• IRAS 16293: A "Magnetic" Tale of Two Cores
• Molecular Cloud Evolution III. Accretion vs. stellar feedback
• Density Power Spectrum of Compressible Hydrodynamic Turbulent Flows
• The Distribution of Pressures in a Supernova-Driven Interstellar Medium. I. Magnetized Medium
• Assessing Radiation Pressure as a Feedback Mechanism in Star-Forming Galaxies
• Analysis of Clumps in Molecular Cloud Models: Mass Spectrum, Shapes, Alignment and Rotation
• Velocity Gradients as a Tracer for Magnetic Fields
• Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
• The Magnetic Field Morphology of the Class 0 Protostar L1157-mm
• On the properties of young multiple stars
• Magnetorotationally-Driven Galactic Turbulence and the Formation of Giant Molecular Clouds
• Radial Profiles of Star Formation in the Far Outer Regions of Galaxy Disks
• Quantifying Observational Projection Effects Using Molecular Cloud Simulations
• Maximally Star-Forming Galactic Disks II. Vertically-Resolved Hydrodynamic Simulations of Starburst Regulation
• Interferometric observations of magnetic fields in forming stars
• Spectral Properties of Compressible Magnetohydrodynamic Turbulence from Numerical Simulations
• Anchoring Magnetic Field in Turbulent Molecular Clouds
• Star formation in unbound giant molecular clouds: the origin of OB associations?
• The statistical properties of stars and their dependence on metallicity
• Past and present star formation in the SMC: NGC 346 and its neighborhood
• Optical polarimetry toward the Pipe nebula: Revealing the importance of the magnetic field
• Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps
• The statistical properties of stars and their dependence on metallicity: the effects of opacity
• The Sizes and Luminosities of Massive Star Clusters
• Magnetic Fields in Diffuse H I and Molecular Clouds
• The Stability of Magnetized Rotating Plasmas with Superthermal Fields
• One Dimensional Dynamical Models of the Carina Nebula Bubble
• ALMA observations of dust polarization and molecular line emission from the Class 0 protostellar source Serpens SMM1
• On the Kennicutt-Schmidt relation of low-metallicity high-redshift galaxies
• Magnetically Dominated Strands of Cold Hydrogen in the Riegel-Crutcher Cloud
• An Excursion-Set Model for the Structure of GMCs and the ISM
• Algorithmic comparisons of decaying, isothermal, supersonic turbulence
• Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
• A Turbulent Origin for Flocculent Spiral Structure in Galaxies
• Tracing interstellar magnetic field using velocity gradient technique: Application to Atomic Hydrogen data
• A method for reconstructing the variance of a 3D physical field from 2D observations: Application to turbulence in the ISM
• The dependence of star formation on initial conditions and molecular cloud structure
• Gravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation
• Supersonic turbulence and structure of interstellar molecular clouds
• Numerical Simulations of Turbulent, Molecular Clouds Regulated by Radiation Feedback Forces I: Star Formation Rate and Efficiency
• A supersonic turbulence origin of Larson's laws
• Probing the evolution of molecular cloud structure II: From chaos to confinement
• Density Probability Distribution Functions in Supersonic Hydrodynamic and MHD Turbulence
• The Average Magnetic Field Strength in Molecular Clouds: New Evidence of Super-Alfvenic Turbulence
• Structure Function Scaling in Compressible Super-Alfvenic MHD Turbulence
• DESPOTIC -- A New Software Library to Derive the Energetics and SPectra of Optically Thick Interstellar Clouds
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• The Fundamentally Different Dynamics of Dust and Gas in Molecular Clouds
• The nonlinear development of the thermal instability in the atomic ISM and its interaction with random fluctuations
• Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation
• Does Magnetic Levitation or Suspension Define the Masses of Forming Stars?
• Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds
• Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman Observations
• The Formation of Star Clusters I: 3D Simulations of Hydrodynamic Turbulence
• Approximations for modelling CO chemistry in GMCs: a comparison of approaches
• Interferometric Mapping of Magnetic Fields in Star-forming Regions I. W51 e1/e2 Molecular Cores
• Interferometric Mapping of Magnetic Fields in Star-forming Regions II. NGC2024 FIR5
• High-accuracy estimation of magnetic field strength in the interstellar medium from dust polarization
• High resolution 21 cm mapping of the Ursa Major Galactic cirrus: power spectra of the high-latitude HI gas
• Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions
• Modes of Star Formation in Finite Molecular Clouds
• Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network
• Accretion and Dynamical Interactions in Small-N Star-Forming Clusters: I. N=5 case
• Sub-Eddington Star-Forming Regions are Super-Eddington: Momentum Driven Outflows from Supersonic Turbulence
• STARFORGE: The effects of protostellar outflows on the IMF
• Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments
• On the use of fractional Brownian motion simulations to determine the 3D statistical properties of interstellar gas
• There is no magnetic braking catastrophe: Low-mass star cluster and protostellar disc formation with non-ideal magnetohydrodynamics
• The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
• Change of Magnetic Field$-$Gas Alignment at Gravity-Driven Alfvénic Transition in Molecular Clouds: Implications for Dust Polarization Observations
• Magnetic Field Strength Maps for Molecular Clouds: A New Method Based on a Polarization - Intensity Gradient Relation
• A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields
• Submillimeter Array Observations of Magnetic Fields in G240.31+0.07: an Hourglass in a Massive Cluster-forming Core
• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• The art of modeling CO, [CI], and [CII] in cosmological galaxy formation models
• CO line emission from galaxies in the Epoch of Reionization
• Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24
• Attenuation caused by a distant Isothermal Turbulent Screen
• From parallel to perpendicular -- On the orientation of magnetic fields in molecular clouds
• The formation and dynamical evolution of young star clusters
• The Effect of Projection on Derived Mass-Size and Linewidth-Size Relationships
• The Angular Momentum of Magnetized Molecular Cloud Cores: A 2D-3D Comparison
• The Stellar Mass Distribution in the Giant Star Forming Region NGC 346
• Magnetic Field Morphology in Interstellar Clouds with the Velocity Gradient Technique
• The shapes of column density PDFs - The importance of the last closed contour
• Unmasking the Supernova Impostors
• Particle Acceleration by MHD Turbulence
• Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media
• A Submillimetre Imaging Polarimeter at the James Clerk Maxwell Telescope
• The dependence of the sub-stellar IMF on the initial conditions for star formation
• Magnetic fields towards Ophiuchus-B derived from SCUBA-2 polarization measurements
• Sub-mm Emission Line Deep Fields: CO and [CII] Luminosity Functions out to z = 6
• Line Profiles of Cores within Clusters: I. The Anatomy of a Filament
• Star Formation in the First Galaxies - II: Clustered Star Formation and the Influence of Metal Line Cooling
• Ubiquitous velocity fluctuations throughout the molecular interstellar medium
• Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
• Density probability distribution functions of diffuse gas in the Milky Way
• The Physical Nature of Neutral Hydrogen Intensity Structure
• On the Power-Law Tail in the Mass Function of Protostellar Condensations and Stars
• Synthetic infrared images and spectral energy distributions of a young low-mass stellar cluster
• Structure of Stationary Strong Imbalanced Turbulence
• A First Look at BISTRO Observations of The $\rho$ Oph-A core
• Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust
• The Interaction of Cosmic Rays with Diffuse Clouds
• The Interstellar Magnetic Field Close to the Sun II
• Evolution of Magnetic Fields in High Mass Star Formation: SMA dust polarization image of the UCHII region G5.89-0.39
• Does the magnetic field suppress fragmentation in massive dense cores?
• Emissivity Statistics in Turbulent, Compressible MHD Flows and the Density-Velocity Correlation
• A method for reconstructing the PDF of a 3D turbulent density field from 2D observations
• Highly Ordered and Pinched Magnetic Fields in the Class 0 Proto-Binary System L1448 IRS 2
• 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
• Extending the Shakura-Sunyaev approach to a strongly magnetized accretion disc model
• The magnetic field and dust filaments in the Polaris Flare
• JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146
• Magnetically-Regulated Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion
• ALMA resolves the hourglass magnetic field in G31.41+0.31
• Star formation in turbulent molecular clouds with colliding flow
• The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds
• The Inability of Ambipolar Diffusion to set a Characteristic Mass Scale in Molecular Clouds
• Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing
• The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region
• Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models
• The structure of molecular clouds and the universality of the clump mass function
• Starburst Galaxies: Why the Calzetti Dust Extinction Law?
• Characteristics of the structure in the Galactic polarized radio background at 350 MHz
• Dense gas without star formation: The kpc-sized molecular disk in 3C326 N
• An Initial Mass Function for Individual Stars in Galactic Disks: I. Constraining the Shape of the IMF
• Turbulent Disks are Never Stable: Fragmentation and Turbulence-Promoted Planet Formation
• Turbulent Mixing in the Interstellar Medium -- an application for Lagrangian Tracer Particles
• A technique for constraining the driving scale of turbulence and a modified Chandrasekhar-Fermi method
• SCUBA polarisation observations of the magnetic fields in the prestellar cores L1498 and L1517B
• The JCMT BISTRO Survey: The Magnetic Field In The Starless Core $\rho$ Ophiuchus C
• Cluster assembly and the origin of mass segregation in the STARFORGE simulations
• Comparing star formation models with interferometric observations of the protostar NGC 1333 IRAS 4A. I. Magnetohydrodynamic collapse models
• Calibrating the Davis-Chandrasekhar-Fermi method with numerical simulations: uncertainties in estimating the magnetic field strength from statistics of field orientations
• Physical Properties of Dense Cores in the Rho Ophiuchi Main Cloud and A Significant Role of External Pressures in Clustered Star Formation
• Magnetic fields in the infrared dark cloud G34.43+0.24
• 2MASS wide field extinction maps: V. Corona Australis
• Trans-Alfvenic Motions in the Taurus Molecular Cloud
• Star Formation in Transient Molecular Clouds
• Dust Polarization Toward Embedded Protostars in Ophiuchus with ALMA. II. IRAS 16293-2422
• Self-gravitating Filament Formation from Shocked Flows: Velocity Gradients across Filaments
• Magnetic fields in star formation: a complete compilation of all the DCF estimations
• JCMT POL-2 and BISTRO Survey observations of magnetic fields in the L1689 molecular cloud
• The Dependence of Star Formation Efficiency on Gas Surface Density
• Magnetic field structure in a high-mass outflow/disk system
• First observations of the magnetic field inside the Pillars of Creation: Results from the BISTRO survey
• CO excitation, molecular gas density and interstellar radiation field in local and high-redshift galaxies
• Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud
• The strength and structure of the magnetic field in the galactic outflow of M82
• Diffusion in supersonic, turbulent, compressible flows
• The Spectral Correlation Function of Molecular Clouds: A Statistical Test for Theoretical Models
• The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XII. The Perseus YSO Population as Observed with IRAC and MIPS
• Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
• Magnetic Fields and Infall Motions in NGC 1333 IRAS 4
• Interferometric mapping of magnetic fields: The ALMA view of the massive star forming clump W43-MM1
• From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
• Supernova Driving. II. Compressive Ratio in Molecular-Cloud Turbulence
• The Carina Nebula and Gum 31 molecular complex: I. Molecular gas distribution, column densities and dust temperatures
• Formation and Collapse of Quiescent Cloud Cores Induced by Dynamic Compressions
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• Spiral shocks and the formation of molecular clouds in a two phase medium
• Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code
• Formation of the Hub-Filament System G33.92+0.11: Local Interplay between Gravity, Velocity, and Magnetic Field
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• The magnetic environment of the Orion-Eridanus superbubble as revealed by Planck
• Evolving Molecular Cloud Structure and the Column Density Probability Distribution Function
• The nature of the ISM in galaxies during the star-formation activity peak of the Universe
• Can the Lyman Continuum leaked out of H II regions explain Diffuse Ionized Gas?
• Evidence for Grain Growth in Molecular Clouds: A Bayesian Examination of the Extinction Law in Perseus
• Do Lognormal Column-Density Distributions in Molecular Clouds Imply Supersonic Turbulence?
• Clustered Star Formation in Magnetic Clouds: Properties of Dense Cores Formed in Outflow-Driven Turbulence
• Gravitational Collapse of Filamentary Magnetized Molecular Clouds
• Molecular Tracers of Turbulent Shocks in Giant Molecular Clouds
• Near-Infrared Imaging Polarimetry of the Serpens Cloud Core: Magnetic Field Structure, Outflows, and Inflows in A Cluster Forming Clump
• Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC+ and comparing with simulation
• Synthetic observations of star formation and the interstellar medium
• Enhanced Core Formation Rate in a Turbulent Cloud by Self-gravity
• Magnetic field properties in star formation: a review of their analysis methods and interpretation
• The JCMT BISTRO Survey: The Distribution of Magnetic Field Strengths towards the OMC-1 Region
• B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main
• Magnetic fields in the early stages of massive star formation as revealed by ALMA
• Three-dimensional extinction mapping using Gaussian random fields
• Magnetic Properties of Star-Forming Dense Cores
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• Demonstration of magnetic field tomography with starlight polarization towards a diffuse sightline of the ISM
• Interpreting the Low Frequency Radio Spectra of Starburst Galaxies: A Pudding of Strömgren Spheres
• 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
• Lyα emission from galaxies in the Epoch of Reionization
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• Non-ideal magnetohydrodynamics vs turbulence I: Which is the dominant process in protostellar disc formation?
• Evaluating the Magnetic Field Strength in Molecular Clouds
• Can magnetized turbulence set the mass scale of stars?
• TurbuStat: Turbulence Statistics in Python
• Cloud formation in the atomic and molecular phase: HI self absorption (HISA) towards a Giant Molecular Filament
• Turbulence Dynamo in Galaxy Clusters
• Near-IR Imaging Polarimetry toward a Bright-Rimmed Cloud: Magnetic Field in SFO 74
• CN Zeeman and dust polarization in a high-mass cold clump
• Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
• The Probability Distribution of Density Fluctuations in Supersonic Turbulence
• Gas shells and magnetic fields in the Orion-Eridanus superbubble
• Non-Gaussian velocity shears in the environment of low mass dense cores
• Turbulent stagnation in a z-pinch plasma
• DR21 Main: A Collapsing Cloud
• Observational Determination of the Turbulent Ambipolar Diffusion Scale and Magnetic Field Strength in Molecular Clouds
• Alignment of Outflows with Magnetic Fields in Cloud Cores
• The Density Distribution in Turbulent Bi-stable Flows
• Magnetic field structure around cores with very low luminosity objects
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• Near-Infrared Polarimetric Adaptive Optics Observations of NGC 1068: A torus created by a hydromagnetic outflow wind
• The IMF as a function of supersonic turbulence
• Cosmic rays across the star-forming galaxy sequence. I: Cosmic ray pressures and calorimetry
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• ALMA Observations of a Quiescent Molecular Cloud in the Large Magellanic Cloud
• Damping of MHD turbulence in partially ionized gas and the observed difference of velocities of neutrals and ions
• A Simple Perspective on the Mass-Area Relationship in Molecular Clouds
• The turbulent fragmentation of the interstellar medium: The impact of metallicity on global star formation
• Dusty Cloud Acceleration by Radiation Pressure in Rapidly Star-Forming Galaxies
• The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence
• MHD Turbulence, Turbulent Dynamo and Applications
• The Magnetic Field of Cloud 3 in L204
• A Catalog of HI Clouds in the Large Magellanic Cloud
• The Radio-FIR correlation: Is MHD Turbulence the Cause?
• Optical/Near-IR Polarization Survey of Sh 2-29: Magnetic Fields, Dense Cloud Fragmentations and Anomalous Dust Grain Sizes
• The density structure of supersonic self-gravitating turbulence
• Effects of initial density profiles on massive star cluster formation in giant molecular clouds
• The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2
• The Magnetic Field Structure in W51A
• Gravity and rotation drag the magnetic field in high-mass star formation
• An Observational Method to Measure the Relative Fractions of Solenoidal and Compressible Modes in Interstellar Clouds
• Simulating the H2 content of high-redshift galaxies
• Numerical simulations of supernova remnants in turbulent molecular clouds
• A Study of starless dark cloud LDN 1570: Distance, Dust properties and Magnetic field geometry
• The balloon-borne large-aperture submillimeter telescope for polarimetry: BLAST-Pol
• Formation of young massive clusters from turbulent molecular clouds
• Effect of dust on Kelvin-Helmholtz instabilities
• ALMA polarimetry measures magnetically aligned dust grains in the torus of NGC 1068
• Maps of Magnetic Field Strength in the OMC-1 using HAWC+ FIR Polarimetric data
• The role of the magnetic field in the fragmentation process: the case of G14.225-0.506
• Direct Evidence for Two-Fluid Effects in Molecular Clouds
• Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud II: A Parameter Study
• Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling
• What is a GMC? Are Observers and Simulators Discussing the Same Star-forming Clouds?
• Polarimetry toward the IRAS Vela Shell. II. Extinction and Magnetic Fields
• A scaling relation for the molecular cloud lifetime in Milky Way-like galaxies
• Gravity Versus Magnetic Fields in Forming Molecular Clouds
• Observations of magnetic fields surrounding LkH$\alpha$ 101 taken by the BISTRO survey with JCMT-POL-2
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• Magnetic Field Structure in Spheroidal Star-Forming Clouds
• Resolved Magnetic Field Mapping of a Molecular Cloud Using GPIPS
• Compressed magnetized shells of atomic gas and the formation of the Corona Australis molecular cloud
• Mid-J CO observations of Perseus B1-East 5: evidence for turbulent dissipation via low-velocity shocks
• Star formation in the filament of S254-S258 OB complex: a cluster in the process of making
• Envelope Expansion with Core Collapse II. Quasi-Spherical Self-Similar Solutions for an Isothermal Magnetofluid
• Distortion of Magnetic Fields in a Starless Core: Near-Infrared Polarimetry of FeSt 1-457
• Does turbulence determine the initial mass function?
• The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament
• Non-ideal magnetohydrodynamics vs turbulence II: Which is the dominant process in stellar core formation?
• Testing Density Wave Theory with Resolved Stellar Populations around Spiral Arms in M81
• The Davis-Chandrasekhar-Fermi Method Revisited
• Relationship between the column density distribution and evolutionary class of molecular clouds as viewed by ATLASGAL
• Tracing Multi-Scale Magnetic Field Structure Using Multiple Chemical Tracers in Giant Molecular Clouds
• Stellar and substellar initial mass function: a model that implements gravoturbulent fragmentation and accretion
• The Effect of Turbulence on Nebular Emission Line Ratios
• Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
• ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
• Dense Gas in a Giant Molecular Filament
• Near-Infrared Imaging Polarimetry of the NGC 2071 Star Forming Region with SIRPOL
• Magnetic Field Properties in High Mass Star Formation from Large to Small Scales - A Statistical Analysis from Polarization Data
• The SOFIA FEEDBACK Legacy Survey: Dynamics and mass ejection in the bipolar HII region RCW 36
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Evidence for Dynamically Important Magnetic Fields in Molecular Clouds
• Hydrodynamical simulations of the decay of high-speed molecular turbulence. II. Divergence from isothermality
• Driven Multifluid MHD Molecular Cloud Turbulence
• Interstellar MHD Turbulence and Star Formation
• The JCMT BISTRO Survey: An 850/450$\mu$m Polarization Study of NGC 2071IR in OrionB
• Formation of the SDC13 Hub-Filament System: A Cloud-Cloud Collision Imprinted on The Multiscale Magnetic Field
• Effects of multiple-scale driving on turbulence statistics
• Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetised molecular cloud cores
• A New Method for Constraining Molecular Cloud Thickness: A study of Taurus, Perseus and Ophiuchus
• On the Origin of the High Column Density Turnover in the HI Column Density Distribution
• The highly variable time evolution of star-forming cores identified with dendrograms
• Rotating filament in Orion B: Do cores inherit their angular momentum from their parent filament?
• Effect of feedback of massive stars in the fragmentation, distribution, and kinematics of the gas in two star forming regions in the Carina Nebula
• Can Sgr A* flares reveal the molecular gas density PDF?
• Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling
• B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): I. The massive filament G11.11-0.12 observed by SOFIA/HAWC+
• First polarimetry results of two candidate high-mass protostellar objects
• High Angular Resolution Measurement of Ion and Neutral Spectra as a Probe of the Magnetic Field Structure in DR21(OH)
• Atomic Chemistry in Turbulent Astrophysical Media II: Effect of the Redshift Zero Metagalactic Background
• A Curved Magnetic field in the ring-like shell of bubble N4
• Dense Regions in Supersonic Isothermal Turbulence
• Dispersion of Observed Position Angles of Submillimeter Polarization in Molecular Clouds
• Submillimeter polarisation and magnetic field properties in the envelopes of proto-planetary nebulae CRL 618 and OH 231.8+4.2
• Magnetic field structure in the Flattened Envelope and Jet in the young protostellar system HH 211
• The seven most massive clumps in W43-Main as seen by ALMA: Dynamical equilibrium and Magnetic Fields
• Rethinking the N(H2)/I(CO) Conversion Factor
• Cosmic Rays and Magnetic Fields in the Core and Halo of the Starburst M82: Implications for Galactic Wind Physics
• Large-scale three-dimensional Gaussian process extinction mapping
• Complex Scattered Radiation Fields and Multiple Magnetic Fields in the Protostellar Cluster in NGC 2264
• Magnetic fields in multiple bright-rimmed clouds in different directions of H II region IC1396 - II
• Effects of Grain Alignment Efficiency on Synthetic Dust Polarization Observations of Molecular Clouds
• Near-Infrared Imaging Polarimetry toward M17 SWex
• The magnetic properties of the protostellar core IRAS 15398-3359
• The magnetic field in the NGC 2024 FIR 5 dense core
• Magnetic field geometry of an unusual cometary cloud Gal 110-13
• Fantastic Striations and Where to Find Them: Origin of Magnetically Aligned Striations in Interstellar Clouds
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• The Magnetic Field in the Milky Way Filamentary Bone G47
• The Balloon-borne Large-Aperture Submillimeter Telescope for Polarization: BLAST-pol
• Insights from Simulations of Star Formation
• The statistical properties of stars at redshift, z=5, compared with the present epoch
• Tracing the Magnetic Field of IRDC G028.23$-$00.19 Using NIR Polarimetry
• Estimations of the magnetic field strength in the torus of AGN using near-infrared polarimetry
• Bayesian inference of three-dimensional gas maps: II. Galactic HI
• An Exploration of the Statistical Signatures of Stellar Feedback
• Distortion of Magnetic Fields in a Starless Core IV: Magnetic Field Scaling on Density and Mass-to-flux Ratio Distribution in FeSt 1-457
• Galactic dust evolution with rapid dust formation in the interstellar medium due to hypersonic turbulence
• Probability distribution functions of gas in M31 and M51
• Galaxy Evolution: Modeling the Role of Non-thermal Pressure in the Interstellar medium
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments II: Star Formation and Pressure Balance in HI-Rich UDGs
• Molecular cloud formation as seen in synthetic Hi and molecular gas observations
• Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds. II. Directly Probing the Ion-neutral Decoupling Scale
• The Photon Dominated Region in the IC 348 molecular cloud
• X-ray spectroscopy of the starburst feedback in 30 Doradus
• Hypersonic Buckshot: Astrophysical Jets as Heterogeneous Collimated Plasmoids
• Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study on Sh2-201 with JCMT SCUBA-2/POL-2
• Comparison of Prestellar Core Elongations and Large-Scale Molecular Cloud Structures in the Lupus I Region
• The Magnetized Environment of the W3(H2O) Protostars
• An Extension of the Athena++ Framework for Fully Conservative Self-Gravitating Hydrodynamics
• Probing the magnetic fields in L1415 and L1389
• Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics?
• Polarization of seven MBM clouds at high galactic latitude
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds III: SLED fitting
• Probing the Turbulent Ambipolar Diffusion Scale in Molecular Clouds with Spectroscopy
• Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement
• The Impact of Unresolved Turbulence on the Escape Fraction of Lyman Continuum Photons
• Magnetic Field and Faraday Rotation Measure in the Turbulent Warm Ionized Medium
• Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
• Study of magnetic field geometry and extinction in Bok globule CB130
• Kinematic signatures of cluster formation from cool collapse in the Lagoon Nebula cluster NGC 6530
• First Sub-pc Sale Mapping of Magnetic Fields in the Vicinity of a Very Low Luminosity Object, L1521F-IRS
• Sink particle radiative feedback in smoothed particle hydrodynamics models of star formation
• Bayesian inference of three-dimensional gas maps: I. Galactic CO
• Observational Diagnostics for Two-Fluid Turbulence in Molecular Clouds As Suggested by Simulations
• HI-H${}_2$ transition: exploring the role of the magnetic field
• The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43
• Long-lived Magnetic-Tension-Driven Modes in a Molecular Cloud
• Magnetic Field Structure of the HH 1-2 Region: Near-Infrared Polarimetry of Point-Like Sources
• Estimation of Magnetic Field Strength in the Turbulent Warm Ionized Medium
• Irregular Magnetic Fields and the Far-Infrared Polarimetry of Dust Emission from Interstellar Clouds
• Understanding the links among magnetic fields, filament, the bipolar bubble, and star formation in RCW57A using NIR polarimetry
• Multifluid magnetohydrodynamic turbulent decay
• Distortion of Magnetic Fields in Barnard 335
• Polarimetric and photometric investigation of a dark globule LDN 1225: distance, extinction law, and magnetic fields
• Mid-J CO Shock Tracing Observations of Infrared Dark Clouds I
• Effects of Galactic Disc Inclination and Resolution on Observed GMC Properties and Larson's Scaling Relations
• Magnetic fields in star-forming systems (II): examining dust polarization, the Zeeman effect, and the Faraday rotation measure as magnetic field tracers
• On the frequencies of circumbinary discs in protostellar systems
• Magnetic Field Structures in Star Forming Regions: Mid-Infrared Imaging Polarimetry of K3-50
• Evolution of the Hub-filament Structures in IC 5146 in the Context of the Energy Balance of Gravity, Turbulence, and Magnetic Field
• Variation of the low-mass end of the stellar initial mass function with redshift and metallicity
• The statistical properties of protostellar discs and their dependence on metallicity
• Alignment of dense molecular core morphology and velocity gradients with ambient magnetic fields
• Magnetic Field Structure of Orion Source I
• Increasing mass-to-flux ratio from the dense core to the protostellar envelope around the Class 0 protostar HH 211
• A correlation between chemistry, polarization and dust properties in the Pipe Nebula starless core FeSt 1-457
• The dependence of stellar properties on initial cloud density
• Velocity centroid gradients for absorbing media
• The Column Density Variance in Turbulent Interstellar Media: A Fractal Model Approach
• Three-dimensional magnetic fields of molecular clouds
• Magnetic Field Structure in Spheroidal Star-Forming Clouds. II. Estimating Field Structure from Observed Maps
• On the grain-size distribution of turbulent dust growth
• Non-ideal MHD turbulent decay in molecular clouds
• On the properties of fractal cloud complexes
• Magnetic Fields and Fragmentation of Filaments in the Hub of California-X
• HOW-MHD: A High-Order WENO-Based Magnetohydrodynamic Code with a High-Order Constrained Transport Algorithm for Astrophysical Applications
• The Role of Magnetic Fields in the Stability and Fragmentation of Filamentary Molecular Clouds: Two Case Studies at OMC-3 and OMC-4
• The Role of Magnetic Fields in Triggered Star Formation of RCW 120
• On the probability distribution function of the mass surface density of molecular clouds I
• Interactions between Gas Dynamics and Magnetic Fields in the Massive Dense Cores of the DR21 Filament
• Modeling Star Formation as a Markov Process in a Supersonic Gravoturbulent Medium
• Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19
• Magnetic fields and outflows in the large Bok globule CB 54
• A Synergy of the Velocity Gradients Technique and the Probability Density Functions for Identifying Gravitational Collapse in Self-Absorbing Media
• Magnetic fields and Star Formation around HII regions: The S235 complex
• Cloud properties across spatial scales in simulations of the interstellar medium
• Type III Societies (Apparently) Do Not Exist
• Distortion of Magnetic Fields in a Starless Core VI: Application of Flux Freezing Model and Core Formation of FeSt 1-457
• A Dynamically Collapsing Core and a Precursor of a Core in a Filament Supported by Turbulent and Magnetic Pressures
• Distortion of Magnetic Fields in BHR 71
• Dust Scattering In Turbulent Media: Correlation Between The Scattered Light and Dust Column Density
• The Dependence of Prestellar Core Mass Distributions on the Structure of the Parental Cloud
• The JCMT BISTRO-2 Survey: The Magnetic Field in the Center of the Rosette Molecular Cloud
• X-raying molecular clouds with a short flare: probing statistics of gas density and velocity fields
• No impact of core-scale magnetic field, turbulence, or velocity gradient on sizes of protostellar disks in Orion A
• On the probability distribution function of the mass surface density of molecular clouds. II
• NGC 7538 IRS1: Interaction of a polarized dust spiral and a molecular outflow
• Star Formation in a Strongly Magnetized Cloud
• The supernova-regulated ISM. IV. A comparison of simulated polarization with Planck observations
• Turbulent magnetic field in the HII region Sh 2-27
• Three-dimensional extinction mapping and selection effects
• The Role of Magnetic Fields in the Formation of the Filamentary Infrared Dark Cloud G11.11-0.12
• Low-Mass Star Forming Cores in the GF9 Filament
• Geometry-Independent Determination of Radial Density Distributions in Molecular Cloud Cores and Other Astronomical Objects
• CO enhancement by magnetohydrodynamic waves; Striations in the Polaris Flare
• Mapping and characterizing magnetic fields in the Rho Ophiuchus-A molecular cloud with SOFIA/HAWC$+$
• Aspect ratios of far-infrared and H i filaments in the diffuse interstellar medium at high Galactic latitudes
• Nonlinear Criterion for the Stability of Molecular Clouds
• CN Zeeman observations of the NGC 2264-C protocluster
• Entropy and Mass Distribution in Disc Galaxies
• Molecular Clouds. Formation and Disruption
• Turbulent Fragmentation and Star Formation
• Energy conserving and well-balanced discontinuous Galerkin methods for the Euler-Poisson equations in spherical symmetry
• An analytical model for the evolution of starless cores I: The constant-mass case
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• DIISC-II: Unveiling the Connections between Star Formation and ISM in the Extended Ultraviolet Disk of NGC 3344
• Long-Term Evolution of Decaying MHD Turbulence in the Multiphase ISM
• A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey
• Kinematics of Subclusters in Star Cluster Complexes: Imprint of their Parental Molecular Clouds
• Lognormal intensity distribution of the FUV continuum background shortward of Ly-alpha
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae II: Rotation and Turbulence
• SOFIA and ALMA Investigate Magnetic Fields and Gas Structures in Massive Star Formation: The Case of the Masquerading Monster in BYF 73
• Multi log-normal density structure in Cygnus-X molecular clouds: A fitting for N-PDF without power-law
• The embedded ring-like feature and star formation activities in G35.673-00.847
• Molecular Line Profiles from a Core Forming in a Turbulent Cloud
• Distortion of Magnetic Fields in the Dense Core CB81 (L1774, Pipe 42) in the Pipe Nebula
• Magnetic field measurement from the Davis-Chandrasekhar-Fermi method employed with Atomic Alignment
• Initial Ionization of Compressible Turbulence
• Prestellar Cores in Turbulent Clouds: Numerical Modeling and Evolution to Collapse
• Magnetic stability of massive star forming clumps in RCW 106
• The JCMT BISTRO-3 Survey: Variation of magnetic field orientations on parsec and sub-parsec scales in the massive star-forming region G28.34+0.06
• Tracing the magnetic field morphology of the LDN 1172/1174 cloud complex
• Near-Infrared Polarization Source Catalog of the Northeastern Regions of the Large Magellanic Cloud
• A self-gravity module for the PLUTO code
• Distortion of Magnetic Fields in the Dense Core SL42 (CrA-E) in the Corona Australis Molecular Cloud Complex
• The Formation of Filaments and Dense cores in the Cocoon Nebula (IC~5146)
• Relative Alignment Between Magnetic Fields and Molecular Gas Structure in Molecular Clouds
• Length-scales and Dynamics of Carina's Western Wall
• Widespread subsonic turbulence in Ophiuchus North 1
• Star-forming environments in smoothed particle magnetohydrodynamics simulations I: Clump extraction and properties
• Gas and star kinematics in cloud-cloud collisions
• A Guide to Comparisons of Star Formation Simulations with Observations
• Turbulence driven by stellar jets, the possibility and the efficiency
• Galactic Traversability: A New Concept for Extragalactic SETI
• Optical polarimetry study of Lambda-Orionis star-forming region
• Jump relations for magnetohydrodynamic shock waves in non-ideal gas flow
• Twisted magnetic field in star formation processes of L1521 F revealed by submillimeter dual band polarimetry using James Clerk Maxwell Telescope
• Magnetic fields in Bok globules: Multi-wavelength polarimetry as tracer across large spatial scales
• The Density-Magnetic Field Relation in the Atomic ISM
• The bound origin of low-mass stellar binaries
• On the Flux-Intensity Relation of Molecular Clouds
• A multi-scale view of the magnetic field morphology in the hot molecular core G31.41+0.31
• Turbulence and galactic structure
• Modeling the Disk (three-phase) Interstellar Medium
• Obtaining strength of magnetic field from E and B modes of dust polarization
• The Relative Importance of Thermal Gas, Radiation, and Magnetic Pressures Around Star-Forming Regions in Normal Galaxies and Dusty Starbursts
• Impeding Turbulence Decay in Self-gravitating Cloud Cores
• The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
• Why take the square root? An assessment of interstellar magnetic field strength estimation methods
• Turbulence in the Star-forming Interstellar Medium: Steps toward Constraining Theories with Observations
• Measuring the spectral index of turbulent gas with deep learning from projected density maps
• Realistic Models for Filling and Abundance Discrepancy Factors in Photoionised Nebulae
• Unveiling the role of magnetic fields in an accreting filament onto a young protocluster
• Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
• Prospects of Turbulence Studies in High-Energy Density Laser-Generated Plasma: Numerical Investigations in Two Dimensions
• Optical polarimetry of HH 135/HH 136
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Analysis of Galactic molecular cloud polarization maps: a review of the methods
• Construction of a far ultraviolet all sky map from an incomplete survey: Application of a deep learning algorithm
• Cosmic Ray Propagation in Turbulent Spiral Magnetic Fields associated with Young Stellar Objects
• Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A
• Multi-scale Dust Polarization and Spiral-like Stokes-I Residual in the Class I Protostellar System TMC-1A
• Contour Analysis Tool: an interactive tool for background and morphology analysis
• A Survey of Magnetic Field Properties in Bok Globules
• Magneto-Gravitational Regulated Streamer Accretion onto a Class 0 Protostellar System
• Infrared polarisation study of Lynds 1340: A case of RNO 8
• An Improved Fit to the Density Distribution in Supersonic Isothermal Turbulence
• Systematic Investigation of Dust and Gaseous CO in 12 Nearby Molecular Clouds