Cloud-Scale Molecular Gas Properties in 15 Nearby Galaxies
arXiv:1805.00937 · doi:10.3847/1538-4357/aac326
Abstract
We measure the velocity dispersion, , and surface density, , of the molecular gas in nearby galaxies from CO spectral line cubes with spatial resolution - pc, matched to the size of individual giant molecular clouds. Combining galaxies from the PHANGS-ALMA survey with targets from the literature, we characterize independent sightlines where CO is detected at good significance. and show a strong positive correlation, with the best-fit power law slope close to the expected value for resolved, self-gravitating clouds. This indicates only weak variation in the virial parameter , which is - for most galaxies. We do, however, observe enormous variation in the internal turbulent pressure , which spans across our sample. We find , , and to be systematically larger in more massive galaxies. The same quantities appear enhanced in the central kpc of strongly barred galaxies relative to their disks. Based on sensitive maps of M31 and M33, the slope of the - relation flattens at , leading to high for a given and high apparent . This echoes results found in the Milky Way, and likely originates from a combination of lower beam filling factors and a stronger influence of local environment on the dynamical state of molecular gas in the low density regime.
arXiv commentAccepted for publication in ApJ. 45 pages, 11 figures, 8 tables, 4 Appendices; key results summarized in Figure 10. Machine-readable table can be downloaded at http://www.astronomy.ohio-state.edu/~sun.1608/datafile3.txt prior to publication. For a brief video describing the main results of this paper, please see https://www.youtube.com/watch?v=-_eL7t1PVq8&t
References in corpus (112)
- Astropy: A Community Python Package for Astronomy
- emcee: The MCMC Hammer
- The CO-to-H2 Conversion Factor
- The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
- The Star Formation Law in Nearby Galaxies on Sub-Kpc Scales
- Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
- The Neutral Atomic Phases of the ISM in the Galaxy
- A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs
- High-Resolution Rotation Curves and Galaxy Mass Models from THINGS
- HyperLEDA. III. The catalogue of extragalactic distances
- The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
- The Relationship Between Gas Content and Star Formation in Molecule-Rich Spiral Galaxies
- Molecular Gas and Star Formation in Nearby Disk Galaxies
- Re-examining Larson's Scaling Relationships in Galactic Molecular Clouds
- The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
- The CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies
- A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies
- A Universal, Local Star Formation Law in Galactic Clouds, Nearby Galaxies, High-Redshift Disks, and Starbursts
- The Resolved Properties of Extragalactic Giant Molecular Clouds
- xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
- The Spitzer Survey of Stellar Structure in Galaxies (S^4G)
- The Star Formation Rate of Supersonic MHD Turbulence
- On the fraction of star formation occurring in bound stellar clusters
- Regulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/Dynamical Equilibrium Model
- COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
- Physical properties of molecular clouds for the entire Milky Way disk
- A General Model for the CO-H2 Conversion Factor in Galaxies with Applications to the Star Formation Law
- Bar-driven Transport of Molecular Gas to Galactic Centers and Its Consequences
- Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
- Bias-free Measurement of Giant Molecular Cloud Properties
- Feedback, Disk Self-regulation and Galaxy Formation
- The Equilibrium State of Molecular Regions in the Outer Galaxy
- What controls star formation in the central 500 pc of the Galaxy?
- The BIMA Survey of Nearby Galaxies (BIMA SONG): I. The Radial Distribution of CO Emission in Spiral Galaxies
- The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud
- The PdBI Arcsecond Whirlpool Survey (PAWS): Environmental Dependence of Giant Molecular Cloud Properties in M51
- The Central Region of Barred Galaxies: Molecular Environment, Starbursts, and Secular Evolution
- The Spitzer Survey of Stellar Structure in Galaxies (SG): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns
- Gravity or Turbulence? The velocity dispersion-size relation
- The PdBI Arcsecond Whirlpool Survey (PAWS). I. A Cloud-Scale/Multi-Wavelength View of the Interstellar Medium in a Grand-Design Spiral Galaxy
- Giant Molecular Clouds in M33 - I. BIMA All Disk Survey
- Dark matter and visible baryons in M33
- The Role of Pressure in GMC Formation
- ALMA Reveals the Molecular Medium Fueling the Nearest Nuclear Starburst
- CO-dark gas and molecular filaments in Milky Way type galaxies
- Three Dimensional Hydrodynamic Simulations of Multiphase Galactic Disks with Star Formation Feedback: I. Regulation of Star Formation Rates
- A Comparative Study of Giant Molecular Clouds in M51, M33 and the Large Magellanic Cloud
- Gas Kinematics on GMC scales in M51 with PAWS: cloud stabilization through dynamical pressure
- The Plateau de Bure + 30m Arcsecond Whirlpool Survey reveals a thick disk of diffuse molecular gas in the M51 galaxy
- A wide-field HI mosaic of Messier 31. II.The disk warp, rotation and the dark matter halo
- Dynamically Driven Evolution of the Interstellar Medium in M51
- Molecular gas in the Andromeda galaxy
- Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model
- Molecular and Atomic Gas in the Local Group Galaxy M33
- Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100pc scales
- A Wide-field High Resolution HI Mosaic of Messier 31: I. Opaque Atomic Gas and Star Formation Rate Density
- Cloud Scale ISM Structure and Star Formation in M51
- Dusty waves on a starry sea: the mid-infrared view of M31
- Molecular Gas and Star Formation in Bars of Nearby Spiral Galaxies
- A Dynamical Model for the Formation of Gas Rings and Episodic Starbursts Near Galactic Centres
- Comparing molecular gas across cosmic time-scales: the Milky Way as both a typical spiral galaxy and a high-redshift galaxy analogue
- Cosmological evolution of atomic gas and implications for 21 cm HI absorption
- The linewidth-size relationship in the dense ISM of the Central Molecular Zone
- The Perils of Clumpfind: The Mass Spectrum of Sub-structures in Molecular Clouds
- The Panchromatic Hubble Andromeda Treasury XI: The Spatially-Resolved Recent Star Formation History of M31
- High Resolution Molecular Gas Maps of M33
- Giant Molecular Clouds in M64
- Vertical Equilibrium, Energetics, and Star Formation Rates in Magnetized Galactic Disks Regulated by Momentum Feedback from Supernovae
- Analytical theory for the initial mass function: III time dependence and star formation rate
- A Portrait of Cold Gas in Galaxies at 60pc Resolution and a Simple Method to Test Hypotheses That Link Small-Scale ISM Structure to Galaxy-Scale Processes
- ALMA Observations of the Antennae Galaxies: I. A New Window on a Prototypical Merger
- Giant Molecular Clouds in M31: I - Molecular Cloud Properties
- A Multi-Transistion CO Study of the "Antennae" Galaxies NGC4038/9
- The Mass Function of Super Giant Molecular Complexes and Implications for Forming Young Massive Star Clusters in the Antennae (NGC 4038/39)
- A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces: I. Cloud-scale Gas Motions
- Resolved Giant Molecular Clouds in Nearby Spiral Galaxies: Insights from the CANON CO (1-0) Survey
- The PdBI Arcsecond Whirlpool Survey (PAWS): Multi-phase cold gas kinematic of M51
- Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way
- Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds
- Probability Distribution Functions OF 12CO(J = 1-0) Brightness and Integrated Intensity in M51: The PAWS View
- Supernova Driving. IV. The Star Formation Rate of Molecular Clouds
- WISDOM Project - II: Molecular gas measurement of the supermassive black hole mass in NGC4697
- The Physical Conditions in a Pre Super Star Cluster Molecular Cloud in the Antennae Galaxies
- Pressure Relations and Vertical Equilibrium in the Turbulent, Multiphase ISM
- A general theory for the lifetimes of giant molecular clouds under the influence of galactic dynamics
- CI and CO in nearby galaxy centers: the bright galaxies NGC1068 (M77), NGC2146, NGC3079, NGC4826 (M64), and NGC7469
- H-alpha Kinematics of the SINGS Nearby Galaxies Survey. II
- The mid-life crisis of the Milky Way and M31
- Giant Molecular Clouds in the Early-Type Galaxy NGC4526
- What can simulated molecular clouds tell us about real molecular clouds?
- Two Populations of Molecular Clouds in the Antennae Galaxies
- The Varying Mass Distribution of Molecular Clouds Across M83
- The X_CO conversion factor from galactic multiphase ISM simulations
- THOR - The HI, OH, Recombination Line Survey of the Milky Way - The pilot study: HI observations of the giant molecular cloud W43
- WISDOM Project - III: Molecular gas measurement of the supermassive black hole mass in the barred lenticular galaxy NGC4429
- Towards the Secondary Bar: Gas Morphology and Dynamics in NGC 4303
- Unveiling the physical properties and kinematics of molecular gas in the Antennae Galaxies (NGC 4038/9) through high resolution CO (J = 3-2) observations
- Thermal Pressure in the Cold Neutral Medium of Nearby Galaxies
- The JCMT Nearby Galaxies Legacy Survey IV. Velocity Dispersions in the Molecular Interstellar Medium in Spiral Galaxies
- Evolution of Structure in Late-type Spiral Galaxies I: Ionized Gas Kinematics in NGC 628
- Gravitational torques imply molecular gas inflow towards the nucleus of M51
- The VIRUS-P Exploration of Nearby Galaxies (VENGA): The Xco Gradient in NGC 628
- Energy budget of forming clumps in numerical simulations of collapsing clouds
- Molecular Gas Velocity Dispersions in the Andromeda Galaxy
- Dense Gas Fraction and Star Formation Efficiency Variations in the Antennae Galaxies
- ALMA CO and VLT/SINFONI H2 observations of the Antennae overlap region: mass and energy dissipation
- The interstellar medium of the Antennae Galaxies
- What is a GMC? Are Observers and Simulators Discussing the Same Star-forming Clouds?
- How galactic environment regulates star formation
- The molecular gas mass of M33
- Molecular Gas Properties in M83 from CO PDFs
- Structured Molecular Gas Reveals Galactic Spiral Arms
Cited by in corpus (195)
- Star Clusters Across Cosmic Time
- The Evolution of the Star-forming Interstellar Medium across Cosmic Time
- The lifecycle of molecular clouds in nearby star-forming disc galaxies
- Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
- The cold interstellar medium of galaxies in the Local Universe
- Distances to PHANGS Galaxies: New Tip of the Red Giant Branch Measurements and Adopted Distances
- PHANGS-ALMA Data Processing and Pipeline
- The Evolution and Origin of Ionized Gas Velocity Dispersion from to with KMOS
- Mapping metallicity variations across nearby galaxy disks
- PHANGS CO kinematics: disk orientations and rotation curves at 150 pc resolution
- Giant Molecular Cloud Catalogues for PHANGS-ALMA: Methods and Initial Results
- Molecular Gas Properties on Cloud Scales Across the Local Star-forming Galaxy Population
- Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies
- Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-Forming Galaxies
- The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters
- EMPIRE: The IRAM 30-m Dense Gas Survey of Nearby Galaxies
- Star clusters near and far; tracing star formation across cosmic time
- The PHANGS-HST Survey: Physics at High Angular resolution in Nearby GalaxieS with the Hubble Space Telescope
- The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS
- New Constraints on the CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies
- Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
- The molecular cloud lifecycle
- Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
- Molecular Cloud Populations in the Context of Their Host Galaxy Environments: A Multiwavelength Perspective
- Low-J CO Line Ratios From Single Dish CO Mapping Surveys and PHANGS-ALMA
- A 50 pc scale view of star formation efficiency across NGC 628
- Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies
- Heart of Darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroids
- AUTO-MULTITHRESH: A General Purpose Automasking Algorithm
- Star Formation Laws and Efficiencies across 80 Nearby Galaxies
- Molecular clouds in the Cosmic Snake normal star-forming galaxy 8 billion years ago
- Radii of Young Star Clusters in Nearby Galaxies
- A model for the formation of stellar associations and clusters from giant molecular clouds
- How Galactic Environment affects the Dynamical State of Molecular Clouds and their Star Formation Efficiency
- The environmental dependence of the X_CO conversion factor
- The Gas-Star Formation Cycle in Nearby Star-Forming Galaxies I. Assessment of Multi-scale Variations
- Physical Processes in Star Formation
- Star cluster formation in the most extreme environments: Insights from the HiPEEC survey
- The art of modeling CO, [CI], and [CII] in cosmological galaxy formation models
- The physics of gas phase metallicity gradients in galaxies
- The integrated properties of the molecular clouds from the JCMT CO(3-2) High Resolution Survey
- Environmental dependence of the molecular cloud lifecycle in 54 main sequence galaxies
- From diffuse gas to dense molecular cloud cores
- Measuring the mixing scale of the ISM within nearby spiral galaxies
- Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
- Ubiquitous velocity fluctuations throughout the molecular interstellar medium
- Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51
- VERTICO: The Virgo Environment Traced In CO Survey
- The Kennicutt-Schmidt Law and Gas Scale Height in Luminous and Ultra-Luminous Infrared Galaxies
- Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
- Which feedback mechanisms dominate in the high-pressure environment of the Central Molecular Zone?
- The SEDIGISM survey: Molecular clouds in the inner Galaxy
- GA-NIFS: Black hole and host galaxy properties of two z6.8 quasars from the NIRSpec IFU
- CO Multi-line Imaging of Nearby Galaxies (COMING). IX. CO(=2-1)/CO(=1-0) line ratio on kiloparsec scales
- CO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project
- A Characteristic Mass Scale in the Mass-Metallicity Relation of Galaxies
- Live Fast, Die Young: GMC lifetimes in the FIRE cosmological simulations of Milky Way-mass galaxies
- Prevalent externally-driven protoplanetary disc dispersal as a function of the galactic environment
- Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
- Comparing the pre-SNe feedback and environmental pressures for 6000 HII regions across 19 nearby spiral galaxies
- The EDGE-CALIFA survey: exploring the role of the molecular gas on the galaxy star formation quenching
- The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
- The First Maps of -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
- Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
- A fundamental test for stellar feedback recipes in galaxy simulations
- Molecular Gas Properties and CO-to-H2 Conversion Factors in the Central Kiloparsec of NGC 3351
- The Physical Drivers and Observational Tracers of CO-to-H2 Conversion Factor Variations in Nearby Barred Galaxy Centers
- CO excitation, molecular gas density and interstellar radiation field in local and high-redshift galaxies
- Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
- The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
- MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey
- A diversity of starburst-triggering mechanisms in interacting galaxies and their signatures in CO emission
- The Resolved Distributions of Dust Mass and Temperature in Local Group Galaxies
- WISDOM Project -- IX Giant Molecular Clouds in the Lenticular Galaxy NGC4429: Effects of Shear and Tidal Forces on Clouds
- WARPFIELD-EMP: The Self-Consistent Prediction of Emission Lines from Evolving HII Regions in Dense Molecular Clouds
- Do Spectroscopic Dense Gas Fractions Track Molecular Cloud Surface Densities?
- After The Fall: Resolving the Molecular Gas in Post-Starburst Galaxies
- The headlight cloud in NGC 628: An extreme giant molecular cloud in a typical galaxy disk
- The EDGE-CALIFA Survey: Exploring the Star Formation Law through Variable Selection
- Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars
- 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
- Dense molecular gas properties on 100 pc scales across the disc of NGC 3627
- Mass Functions of Giant Molecular Clouds and Young Star Clusters in Six Nearby Galaxies
- Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
- The ALMOND Survey: Molecular cloud properties and gas density tracers across 25 nearby spiral galaxies with ALMA
- Variations in the plane across galactic environments in PHANGS galaxies
- A new estimator of resolved molecular gas in nearby galaxies
- Systematic Variations of CO J=2-1/1-0 Ratio in The Barred Spiral Galaxy M83
- Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
- Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloud
- Molecular gas cloud properties at revealed by the superb angular resolution achieved with ALMA and gravitational lensing
- How do different spiral arm models impact the ISM and GMC population?
- A model for the minimum mass of bound stellar clusters and its dependence on the galactic environment
- A scaling relation for the molecular cloud lifetime in Milky Way-like galaxies
- A 2-3 mm high-resolution molecular line survey towards the centre of the nearby spiral galaxy NGC 6946
- Bird's eye view of molecular clouds in the Milky Way: I. Column density and star formation from sub-pc to kpc scales
- Cloud Properties and Correlations with Star Formation in Numerical Simulations of the Three-Phase ISM
- VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies
- Diverse Molecular Structures Across The Whole Star-Forming Disk of M83: High fidelity Imaging at 40pc Resolution
- The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way
- What is the physics behind the Larson mass-size relation?
- An Unbiased CO Survey Toward the Northern Region of the Small Magellanic Cloud with the Atacama Compact Array. I. Overview: CO Cloud Distributions
- CO Multi-line Imaging of Nearby Galaxies (COMING). III. Dynamical effect on molecular gas density and star formation in the barred spiral galaxy NGC 4303
- Comparing the Properties of GMCs in M33 from Simulations and Observations
- The Nuclear Region of NGC1365: Star Formation, Negative Feedback, and Outflow Structure
- Nearby galaxies in the LOFAR Two-metre Sky Survey II. The magnetic field-gas relation
- Properties of giant molecular clouds in the strongly barred galaxy NGC1300
- Mapping electron temperature variations across a spiral arm in NGC 1672
- The organization of cloud-scale gas density structure: high resolution CO vs. 3.6 m brightness contrasts in nearby galaxies
- Kinematics of the molecular interstellar medium probed by Gaia: steep velocity dispersion-size relation, isotropic turbulence, and location-dependent energy dissipation
- Highly turbulent gas on GMC-scales in NGC 3256, the nearest luminous infrared galaxy
- GA-NIFS and EIGER: A merging quasar host at z=7 with an overmassive black hole
- The turbulent gas structure in the centers of NGC253 and the Milky Way
- WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
- Star Cluster Classification using Deep Transfer Learning with PHANGS-HST
- PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction,
- Duality in spatially resolved star-formation relations in local LIRGs
- On the initial mass-radius relation of stellar clusters
- SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
- Kinematic analysis of the super-extended HI disk of the nearby spiral galaxy M83
- The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
- Molecular gas and star formation in nearby starburst galaxy mergers
- CO Excitation and its Connection to Star Formation at 200 pc in NGC 1365
- Relationship between the Line Width of the Atomic and Molecular ISM in M33
- WISDOM Project -- XV. Giant Molecular Clouds in the Central Region of the Barred Spiral Galaxy NGC 5806
- Far and extreme UV radiation feedback in molecular clouds and its influence on the mass and size of star clusters
- ALMA Observations of Giant Molecular Clouds in the Starburst Dwarf Galaxy Henize 2-10
- PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
- The molecular gas resolved by ALMA in the low-metallicity dwarf merging galaxy Haro 11
- WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
- Testing for Dark Matter in the Outskirts of Globular Clusters
- Binary progenitor systems for Type Ic supernovae
- Star cluster formation and feedback in different environments of a Milky Way-like galaxy
- On the Beam Filling Factors of Molecular Clouds
- Instability analysis for spiral arms of local galaxies: M51, NGC3627 and NGC628
- Bayesian inference of three-dimensional gas maps: I. Galactic CO
- Bird's eye view of molecular clouds in the Milky Way: II. Cloud kinematics from sub-pc to kpc scales
- CO(2-1)/CO(1-0) line ratio on 100 parsec scale in the nearby barred galaxy NGC1300
- WISDOM project -- XI. Star Formation Efficiency in the Bulge of the AGN-host Galaxy NGC 3169 with SITELLE and ALMA
- Virial Clumps in Central Molecular Zone Clouds
- PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
- Building the molecular cloud population: the role of cloud mergers
- A superluminous supernova in high surface density molecular gas within the bar of a metal-rich galaxy
- A 3 mm Spectral Line Survey toward the Barred Spiral Galaxy NGC 3627
- The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS)
- The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
- Theoretical modelling of two-component molecular discs in spiral galaxies
- Understanding the secular evolution of NGC 628 using UVIT
- High-resolution APEX/LAsMA CO and CO (3-2) observation of the G333 giant molecular cloud complex : II. Survival and gravitational collapse of dense gas structures under feedback
- JWST/NIRSpec and MIRI observations of an expanding, jet-driven bubble of warm H in the radio galaxy 3C 326 N
- Efficient radial migration by giant molecular clouds in the first several hundred Myr after the stellar birth
- Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
- SMA Observations of Extended Emission in Interacting Galaxy NGC 3627
- The Age Evolution of the Radio Morphology of Supernova Remnants
- The HASHTAG project I. A Survey of CO(3-2) Emission from the Star Forming Disc of M31
- Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
- The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties
- Sub-kiloparsec empirical relations and excitation conditions of HCN and HCO+ J=3-2 in nearby star-forming galaxies
- A nearly constant CN/HCN line ratio in nearby galaxies: CN as a new tracer of dense gas
- Feedback in Forming Star Clusters: The Mass-Radius Relation and Mass Function of Molecular Clumps in the Large Magellanic Cloud
- CO Multi-line Imaging of Nearby Galaxies (COMING). X. Physical conditions of molecular gas and the local SFR-Mass relation
- Extreme giant molecular clouds in the luminous infrared galaxy NGC 3256
- First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
- When Gas Dynamics Decouples from Galactic Rotation: Characterizing ISM Circulation in Disk Galaxies
- Molecular Line Ratio Diagnostics Along the Radial Cut and Dusty UV-bright Clumps in a Spiral Galaxy NGC 0628
- Is this an Early Stage Merger? A Case Study on Molecular Gas and Star Formation Properties of Arp 240
- FEASTS Combined with Interferometry. III. The Low Column Density HI Around M51 and Possibility of Turbulent-mixing Gas Accretion
- Does the HCN/CO ratio trace the star-forming fraction of gas? I. A comparison with analytical models of star formation
- Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS
- Dense gas scaling relations at kiloparsec scales across nearby galaxies with the ALMA ALMOND and IRAM 30m EMPIRE surveys
- A sensitive, high-resolution, wide-field IRAM NOEMA CO(1-0) survey of the very nearby spiral galaxy IC 342
- A Giant Molecular Cloud Catalog in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
- Molecular clouds in M51 from high-resolution extinction mapping
- The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
- Inadequate turbulent support in low-metallicity molecular clouds
- Giant molecular clouds and their Type classification in M74: Toward understanding star formation and cloud evolution
- Measuring 60-pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA
- Modeling the Mass Distribution and Gravitational Potential of Nearby Disk Galaxies: Implications for the ISM Dynamical Equilibrium
- Anisotropy of random motions of gas in Messier 33
- The magnetic field in the Flame nebula
- Unveiling the gravitationally unstable disc of a massive star-forming galaxy using NOEMA and MUSE
- Do Post-Starburst Galaxies Host Compact Molecular Gas Reservoirs?
- A 260 pc resolution ALMA map of HCN(1-0) in the galaxy NGC 4321
- Effects of CO-dark Gas on Measurements of Molecular Cloud Stability and the Size-Linewidth Relationship
- The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
- The Arp 240 Galaxy Merger: A Detailed Look at the Molecular Kennicutt-Schmidt Star Formation Law on Sub-kpc Scales
- SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
- Does the HCN/CO ratio trace the star-forming fraction of gas? II. Variations in CO and HCN Emissivity
- AGN feeding along a one-armed spiral in NGC 4593: A study using ALMA CO(2-1) observations
- Molecular cloud matching in CO and dust in M33 II. Physical properties of giant molecular clouds
- Molecular Clouds at the Edge of the Galaxy I. Variation of CO J=2-1/1-0 Line Ratio
- VERTICO IX: Signatures of environmental processing of the gas in Virgo cluster spiral galaxies through mapping of CO isotopologues
- Spatially Resolved Star Formation relations in local LIRGs along the complete merger sequence
- On the scale-height of the molecular gas disc in Milky Way-like galaxies
- Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations