Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality

Abstract

Using galaxy group/cluster catalogs created from the Sloan Digital Sky Survey Data Release 7, we examine in detail the specific star formation rate (SSFR) distribution of satellite galaxies and its dependence on stellar mass, host halo mass, and halo-centric radius. All galaxies, regardless of central-satellite designation, exhibit a similar bimodal SSFR distribution, with a strong break at SSFR ~ 10^-11 yr^-1 and the same high SSFR peak; in no regime is there ever an excess of galaxies in the `green valley'. Satellite galaxies are simply more likely to lie on the quenched (`red sequence') side of the SSFR distribution. Furthermore, the satellite quenched fraction excess above the field galaxy value is nearly independent of galaxy stellar mass. An enhanced quenched fraction for satellites persists in groups with halo masses down to 3 x 10^11 Msol and increases strongly with halo mass and toward halo center. We find no detectable quenching enhancement for galaxies beyond ~2R_vir around massive clusters once these galaxies have been decomposed into centrals and satellites. These trends imply that (1) galaxies experience no significant environmental effects until they cross within ~R_vir of a more massive host halo, (2) after this, star formation in active satellites continues to evolve in the same manner as active central galaxies for several Gyrs, and (3) once begun, satellite star formation quenching occurs rapidly. These results place strong constraints on satellite-specific quenching mechanisms, as we will discuss further in companion papers.

13 pages, 6 figures. Accepted for publication in MNRAS, updated to match published version

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• VERTICO VI: Cold-gas asymmetries in Virgo cluster galaxies
• Investigating early-type galaxy evolution with a multi-wavelength approach. III. Insights from SPH simulations with chemo-photometric implementation
• Backsplash galaxies and their impact on galaxy evolution: a three-stage, four-type perspective
• SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• The XXL survey: XLII. Detection and characterization of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety
• Smaller stellar disc scale lengths in rich environments
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Bimodality of Galaxy Disk Central Surface Brightness Distribution in the Spitzer 3.6 micron band
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• Star Formation Properties of Sloan Digital Sky Survey BOSS Void Galaxies in the Hyper Suprime-Cam Survey
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• The co-evolution of strong AGN and central galaxies in different environments
• ALMA-JELLY I: High Resolution CO(2-1) Observations of Ongoing Ram Pressure Stripping in NGC 4858 Reveal Asymmetrical Gas Tail Formation and Fallback
• The Influence of the Dynamic State of Galaxy Clusters on Segregation Phenomena and Velocity Dispersion Profiles
• Identification of 4876 Bent-Tail Radio Galaxies in the FIRST Survey Using Deep Learning Combined with Visual Inspection
• The Origin of Star Formation in Early-type Galaxies Inferred from Spatially Resolved Spectroscopy
• Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• Galaxy clusters and their outskirts: the "red sequence", star formation rate, stellar mass
• The Occurrence of Compact Groups of Galaxies Through Cosmic Time
• Optimizing high redshift galaxy surveys for environmental information
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• The Evolution of Brightest Cluster Galaxies in the Nearby Universe II: The star-formation activity and the Stellar Mass from Spectral Energy Distribution
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• The recent star formation history of NGC 628 on resolved scales
• A 100 kpc Ram Pressure Tail Trailing the Group Galaxy NGC 2276
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• The impact of environment on the lives of disk galaxies as revealed by SDSS-IV MaNGA
• Stripping of the Hot Gas Halos in Member Galaxies of Abell 1795
• Unraveling emission line galaxy conformity at z~1 with DESI early data
• Red Dragon: A Redshift-Evolving Gaussian Mixture Model for Galaxies
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Tracing the green valley with entropic thresholding
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Environmental effects on associations of dwarf galaxies
• Digging deeper into NGC\,6868 I: stellar population
• The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
• ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters
• Satellites and central galaxies in SDSS: the influence of interactions on their properties
• Quenched galaxies in clusters of galaxies and their outskirts
• Spatially resolved stellar populations and emission lines properties in nearby galaxies with J-PLUS -- I. Method and first results for the M101 group
• Cosmic Pathways for Compact Groups in the Milli-Millennium Simulation
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Searching for Spectroscopic Signatures of Ongoing Quenching in SDSS Galaxies
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• AGB populations in post-starburst galaxies
• Compact groups of galaxies in GAMA -- Probing the densest minor systems at intermediate redshifts
• The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
• The VANDELS Survey: Star formation and quenching in two over-densities at 3 < z < 4
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• Post-processing of galaxies due to major cluster mergers I. hints from galaxy colours and morphologies
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Boosting the evolutionary picture of Cl 0024+17 and MS 0451-03: A case study at intermediate-redshift
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
• Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
• ELG$\times$LRG distribution through dark matter halo dynamics
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• ZTF SN Ia DR2: Impact of the galaxy cluster environment on the stretch distribution of Type Ia supernovae
• Assessing the connection between galactic conformity and assembly-type bias
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
• The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
• The Way to Quench: Galaxy evolution in Abell 2142
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• Compact groups from semi-analytical models of galaxy formation -- VI: Evolution of the two first-ranked galaxies
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• The kinematic imprinting of environmental quenching in $z<0.2$ galaxies
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Galaxy disc central surface brightness distribution in the optical and near-infrared bands
• The formation of blue cluster in local Universe
• Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Galaxy quenching across the Cosmic Web: disentangling mass and environment with SDSS DR18
• Virgo Filaments VI: H$\alpha$ clumps in the filaments around the Virgo galaxy cluster
• The Optical Properties of Host Galaxies of Radio Sources in the Coma Cluster