Ram Pressure Stripping of Spiral Galaxies in Clusters

Abstract

We use 3-dimensional SPH/N-BODY simulations to study ram pressure stripping of gas from spiral galaxies orbiting in clusters. We find that the analytic expectation of Gunn & Gott (1972) relating the gravitational restoring force provided by the disk to the ram pressure force, provides a good approximation to the radius that gas will be stripped from a galaxy. However, at small radii it is also important to consider the potential provided by the bulge component. A spiral galaxy passing through the core of a rich cluster such as Coma, will have its gaseous disk truncated to $\sim 4$ kpc, thus losing $\sim 80$ of its diffuse gas mass. The timescale for this to occur is a fraction of a crossing time $\sim 10^7$ years. Galaxies orbiting within poorer clusters, or inclined to the direction of motion through the intra-cluster medium will lose significantly less gas. We conclude that ram-pressure alone is insufficient to account for the rapid and widespread truncation of star-formation observed in cluster galaxies, or the morphological transformation of Sab's to S0's that is necessary to explain the Butcher-Oemler effect.

8 pages, 7 figures, to be published in MNRAS. Levels added/corrected on figures 3, 4 and 5

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• CO($J$=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array
• Radial Color Gradients in K+A Galaxies in Distant Clusters of Galaxies
• The ESO Nearby Abell Cluster Survey IX. The morphology-radius and morphology-density relations in rich galaxy clusters
• DETECTIFz galaxy groups in the REFINE survey -- 1. Group detection and quenched fraction evolution at $z<2.5$
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• Caught in the act: Cluster `k+a' galaxies as a link between spirals and S0s
• The Evolution of Galaxies in and around Clusters at High-Redshift
• The nature of the dwarf population in Abell 868
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• A Spitzer Study of Pseudobulges in S0 Galaxies : Secular Evolution of Disks
• Quiescent galaxies in a virialized cluster at redshift 2: Evidence for accelerated size-growth
• The Three Hundred project: Galaxy groups do not survive cluster infall
• The Evolution of [OII] Emission from Cluster Galaxies
• The dynamical state of galaxy groups and their luminosity content
• A Virgo high-resolution Halpha kinematical survey: I. NGC 4438
• A jolt to the system: ram pressure on low-mass galaxies in simulations of the Local Group
• ROGER: Reconstructing Orbits of Galaxies in Extreme Regions using machine learning techniques
• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• Galaxy Collisions - Dawn of a New Era
• Significant enhancement of ${\mathrm{H}}_2$ formation in disk galaxies under strong ram pressure
• NGC 3314a/b and NGC 3312: Ram pressure stripping in Hydra I Cluster substructure
• The evolution of dwarf galaxies in the Coma supercluster
• Investigating the Projected Phase Space of Gaussian and Non-Gaussian Clusters
• A Machine Learning Approach to Measuring the Quenched Fraction of Low-Mass Satellites Beyond the Local Group
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• Clustercentric distance or local density? It depends on galaxy morphology
• Abell 2384: the galaxy population of a cluster post-merger
• Evolution of Late-type Galaxies in a Cluster Environment: Effects of High-speed Multiple Encounters with Early-type Galaxies
• Multicolor Surface Photometry of Lenticulars I. The Data
• Anisotropic infall in the outskirts of OmegaWINGS galaxy clusters
• Ram pressure stripping of HI-rich galaxies infalling into massive clusters
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• The galaxy population within the virial radius of the Perseus cluster
• Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902
• The trajectories of galaxies in groups: mass loss and preprocessing
• The Effect of Environment on Galaxy Spiral Arms, Bars, Concentration, and Quenching
• Evolutionary Synthesis Models for the Formation of S0 Galaxies in Clusters
• The present-day gas content of simulated field dwarf galaxies
• Environmental effects on the growth of super massive black holes and AGN feedback
• The evolution of star formation activity in galaxy groups
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Effects of galaxy environment on merger fraction
• WALLABY Pilot Survey: First Look at the Hydra I Cluster and Ram Pressure Stripping of ESO 501-G075
• Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim 1.4$
• Effects of environment on sSFR profiles of late-type galaxies in the CALIFA survey
• Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
• Integrated field spectroscopy of E+A (post-starburst) galaxies with the Kyoto3DII
• It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
• Ram pressure stripping of the multiphase ISM: a detailed view from TIGRESS simulations
• The galaxy population of the complex cluster system Abell 3921
• Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• The environmental dependence of rapidly-quenching and rejuvenating galaxies
• The Kinematics of Cluster Galaxies via Velocity Dispersion Profiles
• HI gas content of SDSS galaxies revealed by ALFALFA: implications for the mass-metallicity relation and the environmental dependence of HI in the local Universe
• Kinematics of cluster galaxies and their relation to galaxy evolution
• When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath$z\gtrsim 1$
• Star forming galaxies in the AKARI Deep Field South: identifications and SEDs
• The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems
• Morphological Dependence of Star Formation Properties for the Galaxies in the Merging Galaxy Cluster A2255
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• Ram pressure stripping: An analytical approach
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Star Formation in Partially Gas-Depleted Spiral Galaxies
• Ram-Ppressure Effects on Dense Molecular Arms in the Central Regions of Spiral Galaxies by Intracluster Medium
• Compact star-forming galaxies preferentially quenched to become PSBs in $z<1$ clusters
• The HI content of elliptical and lenticular galaxies with recent star formation
• The role of the Rayleigh-Taylor instability in ram pressure stripped disk galaxies
• Witnessing the star-formation quenching in $L_{\ast }$ ellipticals
• Faint galaxy population in clusters: X-ray emission, cD halos and projection effects
• The strong environmental dependence of black hole scaling relations
• Characteristic mass in galaxy quenching: environmental versus internal effects
• C IV absorbers tracing cool gas in dense galaxy group/cluster environments
• Chemo-dynamical simulations of dwarf galaxy evolution
• CO in Hickson Compact Group galaxies with enhanced warm \htwo\ emission: Evidence for galaxy evolution?
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Impact of cosmic filaments on the gas accretion rate of dark matter halos
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• Spitzer IRAC Low Surface Brightness Observations of the Virgo Cluster
• Large Molecular Gas Reservoirs in Star Forming Cluster Galaxies
• SITELLE Hα Imaging Spectroscopy of z~0.25 Clusters: Emission Line Galaxy Detection and Ionized Gas Offset in Abell 2390 & Abell 2465
• Exploring Galaxy Evolution Time-Scales in Clusters: Insights from the Projected Phase Space
• Evolution of the gas mass fraction in galaxy clusters
• Ram Pressure Stripping and ISM disc Truncation : Prediction vs. Observation
• The Effect of Halo Mass on the HI Content of Galaxies in Groups and Clusters
• Internal kinematics of spiral galaxies in distant clusters III. Velocity fields from FORS2/MXU spectroscopy
• Spatially-Resolved Medium Resolution Spectroscopy of an Interacting E+A (post-starburst) System with the Subaru telescope
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• The imprint of the thick stellar disc in the mid-plane of three early-type edge-on galaxies in the Fornax cluster
• NGC 1436: the making of a lenticular galaxy in the Fornax cluster
• Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• Tidal stripping as a test of satellite quenching in redMaPPer clusters
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2: I.-- Survey description, data analysis, and star formation and AGN activity in the highest density regions
• Blasting away a dwarf galaxy: The "tail" of ESO 324-G024
• Ram pressure stripping of the hot gaseous haloes of galaxies using the k-epsilon sub-grid turbulence model
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) II: reliability of projected phase-space in our understanding of galaxy populations
• Gas stripping and mixing in galaxy clusters: A numerical comparison study
• Diagnostic diagrams for ram-pressure stripped candidates
• Spatially Resolved Spectroscopy of Passive Spiral Galaxies
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• Star formation histories of Coma Cluster galaxies matched to simulated orbits hint at quenching around first pericenter
• Chromodynamical Analysis of Lenticular Galaxies using Globular Clusters and Planetary Nebulae
• Discovery of Globular Clusters in the Proto-Spiral NGC2915: Implications for Hierarchical Galaxy Evolution
• The Large-scale Effect of Environment on Galactic Conformity
• Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies
• Ram pressure stripping in clusters: Gravity can bind the ISM but not the CGM
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• A new analytic ram pressure profile for satellite galaxies
• Disentangling the role of environmental processes in galaxy clusters
• Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
• Evolution of the anti-truncated stellar profiles of S0 galaxies since $z=0.6$ in the SHARDS survey: II - Structural and photometric evolution
• Photometric observations of Southern Abell Cluster Redshifts Survey Clusters: Structure of galaxies in the inner region of clusters of galaxies
• A Search for Young Stars in the S0 Galaxies of a Super-Group at z=0.37
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• Colour gradients in cluster ellipticals at z~1.4: the hidden content of the galaxy central regions
• Survival of Massive Star-forming Galaxies in Cluster Cores Drives Gas-Phase Metallicity Gradients : The Effects of Ram Pressure Stripping
• From haloes to galaxies. III. The gas cycle of local galaxy populations
• ALMA-JELLY I: High Resolution CO(2-1) Observations of Ongoing Ram Pressure Stripping in NGC 4858 Reveal Asymmetrical Gas Tail Formation and Fallback
• Probing the link between quenching and morphological evolution
• Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) III: galaxy evolution patterns in projected phase space around massive X-ray clusters
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• Young Nuclei in Dwarf Elliptical Galaxies
• Smaller stellar disc scale lengths in rich environments
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• J-PLUS: the impact of bars on quenching time-scales in nearby green valley disc galaxies
• Critical Stellar Central Densities Drive Galaxy Quenching in the Nearby Universe
• Morphology, color-magnitude and scaling relations of galaxies in Abell 426
• Constraining the three-dimensional orbits of galaxies under ram pressure stripping with convolutional neural networks
• A general approach to quenching and galactic conformity
• The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
• Dorado and its member galaxies. III. Mapping star formation with FUV imaging from UVIT
• Evolution of 3-dimensional Shape of Passively Evolving and Star-forming Galaxies at $z<1$
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• Origin of optically passive spiral galaxies with dusty star-forming regions: Outside-in truncation of star formation?
• Effects of environment on stellar metallicity profiles of late-type galaxies in the CALIFA survey
• The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• A Multi-Wavelength Study of Low Redshift Cluster of Galaxies II. Environmental Impact on Galaxy Growth
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Quantifying galactic morphological transformations in the cluster environment
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• The Impact of Disturbed Galaxy Clusters on the Kinematics of Active Galactic Nuclei
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Galaxy Groups: Proceedings from a Swinburne University Workshop
• Photoelectric heating effects on the evolution of luminous disk galaxies
• Quantitative measure of evolution of bright cluster galaxies at moderate redshifts
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• Mid-IR Enhanced Galaxies in the Coma & Virgo Cluster: lenticulars with a high star formation rate
• Clustering properties and halo masses for central galaxies in the local Universe
• Gas in Groups and Clusters of Galaxies
• The Three Hundred Project: The stellar angular momentum evolution of cluster galaxies
• The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
• Anomalous Star-Formation Activity of Less-Luminous Galaxies in Cluster Environment
• New X-ray Clusters in the EMSS II: Optical Properties
• The collaborative effect of ram pressure and merging on star formation and stripping fraction
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• Star Formation Histories of Dwarf Spheroidal and Dwarf Elliptical Galaxies in the Local Universe
• Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
• An effective model for the tidal disruption of satellites undergoing minor mergers with axisymmetric primaries
• Central Concentration of Asymmetric Features in Post-starburst Galaxies at $z\sim 0.8$
• A new way to constrain the densities of intra-group medium in groups of galaxies with convolutional neural networks
• SG1120-1202: Mass-Quenching as Tracked by UV Emission in the Group Environment at z=0.37
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• An analytical model to kinematically identify thin discs in MaNGA galaxies
• Implications of the mild gas motion found with Hitomi in the core of the Perseus cluster
• Evolved galaxies in high-density environments across $2.0\le z<4.2$ using the ZFOURGE survey
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Does a Galaxy Fly?
• Morphologically-Identified Merging Galaxies in the SWIRE Fields
• Asymmetry at Low Surface Brightness as an Indicator of Environmental Processes in the Fornax Cluster
• The Sharpest Ultraviolet view of the star formation in an extreme environment of the nearest Jellyfish Galaxy IC 3418
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies
• Dipole Distortions in the Intergalactic Medium
• Photometric and Spectroscopic Study of Abell 0671
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• A Lack of Evidence for Global Ram-pressure Induced Star Formation in the Merging Cluster Abell 3266
• The Competing Influence of Ram Pressure and Tidal Interaction in NGC 2276
• Keys to Cosmology - Clusters of Galaxies
• Extragalactic globular cluster near-infrared spectroscopy: I. Integrated near-infrared spectra of Centaurus A/NGC 5128
• Clustering and physical properties of AGN and Star-Forming Galaxies at fixed stellar mass: does assembly bias have a role in AGN activity?
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• ESO 137-002: a large spiral undergoing edge-on ram-pressure stripping with little star formation in the tail
• Radar-Chart Analysis of Star-Formation Quenching Stages Across Circular Velocity Curve Classes in Nearby CALIFA Galaxies
• Observing Cluster Galaxies and their Progenitors with JDEM
• Initial Investigations of the Outskirts of XLSSC 122
• Morphologies for DECaLS Galaxies through a combination of non-parametric indices and machine learning methods: A comprehensive catalog using the Galaxy Morphology Extractor (galmex) code
• Multi-Object Spectroscopy of Galaxy Clusters at $z\sim 0.95$ in Ultra Deep Survey Field with Different Star-formation Properties and Large-scale Environments