The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters

Abstract

We have measured the equivalent width of the H-alpha emission line for 11006 galaxies brighter than M_b=-19 (LCDM) at 0.05<z<0.1 in the 2dF Galaxy Redshift Survey (2dF), in the fields of seventeen known galaxy clusters. The limited redshift range ensures that our results are insensitive to aperture bias, and to residuals from night sky emission lines. We use these measurements to trace mustar, the star formation rate normalized to Lstar, as a function of distance from the cluster centre, and local projected galaxy density. We find that the distribution of mustar steadily skews toward larger values with increasing distance from the cluster centre, converging to the field distribution at distances greater than ~3 times the virial radius. A correlation between star formation rate and local projected density is also found, which is independent of cluster velocity dispersion and disappears at projected densities below ~1 galaxy (brighter than M_b=-19) per Mpc^2. This characteristic scale corresponds approximately to the mean density at the cluster virial radius. The same correlation holds for galaxies more than two virial radii from the cluster centre. We conclude that environmental influences on galaxy properties are not restricted to cluster cores, but are effective in all groups where the density exceeds this critical value. The present day abundance of such systems, and the strong evolution of this abundance, makes it likely that hierarchical growth of structure plays a significant role in decreasing the global average star formation rate. Finally, the low star formation rates well beyond the virialised cluster rule out severe physical processes, such as ram pressure stripping of disk gas, as being completely responsible for the variations in galaxy properties with environment.

MNRAS, post-referee version resubmitted March 19 Replaced March 21 with full author list

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• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• VIS3COS: III. environmental effects on the star formation histories of galaxies at z~0.8 seen in [OII], H$\delta$, and Dn4000
• BUDHIES IV: Deep 21-cm neutral Hydrogen, optical and UV imaging data of Abell 963 and Abell 2192 at z $\simeq$ 0.2
• Inter-cluster Filaments of Galaxies Programme: Pilot Study Survey and Results
• LoCuSS: Shedding New Light on the Massive Lensing Cluster Abell 1689 - The View From Herschel
• The environment of AGN dwarf galaxies at z$\sim$0.7 from the VIPERS survey
• The miniJPAS survey: The role of group environment in quenching the star formation
• Galaxy star formation in different environments
• The influence of angular momentum and environment on the HI gas of late-type galaxies
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• The Cosmic Web and galaxy evolution around the most luminous X-ray cluster: RXJ1347.5-1145
• ACCESS III: The Nature of Star Formation in the Shapley Supercluster
• ISO's Contribution to the Study of Clusters of Galaxies
• Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering
• Galaxy And Mass Assembly (GAMA): Bivariate functions of H$\alpha$ star forming galaxies
• The Local Cluster Survey I: Evidence of Outside-In Quenching in Dense Environments
• Low and High Surface Brightness Galaxies at Void Walls
• The First Mid-IR View of the Star-forming Properties of Nearby Galaxy Groups
• The environment and characteristics of low redshift galaxies detected by the Herschel-ATLAS
• Evolution of Group Galaxies from the First Red-Sequence Cluster Survey
• The luminosity function of galaxies to $M_{BgVriz}\sim -14$ in $z\sim 0.3$ clusters
• The Morphological decomposition of Abell A868
• Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
• Recent star formation in clusters of galaxies: extreme compact starbursts in A539 and A634
• U-band photometry of 17 WINGS clusters
• The Variation of the Galaxy Luminosity Function with Group Properties
• The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• An H alpha survey of cluster galaxies V: cluster - field comparison for early-type galaxies
• The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7
• A universal correlation between star-formation activity and molecular gas properties across environments
• Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
• The Variation of Galaxy Morphological Type with the Shear of Environment
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).VI. Environmental quenching on HII region scales
• The stellar populations of early-type galaxies -- II. The effects of environment and mass
• H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
• The galaxy morphology-density relation in the EAGLE simulation
• Tully-Fisher analysis of the multiple cluster system Abell 901/902
• The evolution of the bi-modal colour distribution of galaxies in SDSS groups
• ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
• X-ray Groups of Galaxies at 0.5<z<1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Galaxy evolution in nearby groups. II. Galaxy evolution in nearby loose groups. II. Photometric and kinematic characterization of USGC U268 and USGC U376 group members in the Leo cloud
• Stellar Mass and Velocity Functions of Galaxies: Backward evolution and the fate of Milky Way siblings
• Deep spectroscopy of nearby galaxy clusters: II. The Hercules cluster
• Halo models of HI selected galaxies
• Shaping physical properties of galaxy subtypes in the VIPERS survey: environment matters
• The Effect of Environment on Milky Way-mass galaxies in a Constrained Simulation of the Local Group
• Local and large-scale effects on the astrophysics of void-galaxies
• The Role of Galaxy Interaction in Environmental Dependence of the Star Formation Activity at z~1.2
• Anisotropic infall in the outskirts of OmegaWINGS galaxy clusters
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• The Fornax3D project: Environmental effects on the assembly of dynamically cold disks in Fornax cluster galaxies
• The galaxy population within the virial radius of the Perseus cluster
• Clustercentric distance or local density? It depends on galaxy morphology
• The colors of bulges and disks in the core and outskirts of galaxy clusters
• The evolution of star formation activity in galaxy groups
• The Comoving Infrared Luminosity Density: Domination of Cold Galaxies across 0<z<1
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• Effects of galaxy environment on merger fraction
• AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: mid-infrared view of transition galaxies
• How typical is the Coma cluster?
• At the Vigintennial of the Butcher-Oemler Effect
• Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
• Analytical halo model of galactic conformity
• On the accretion of a new group of galaxies onto Virgo: II. The effect of pre-processing on the stellar population content of dEs
• The effects of stellar populations on galaxy scaling relations in the 6dF Galaxy Survey
• Optical Galaxy Clusters in the Deep Lens Survey
• Nature vs. nurture in the low-density environment: structure and evolution of early-type dwarf galaxies in poor groups
• The role of stellar mass and environment for cluster blue fraction, AGN fraction and star-formation indicators from a targeted analysis of Abell 1691
• The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions
• NUV signatures of environment driven galaxy quenching in SDSS groups
• Revealing Dust Obscured Star Formation in CLJ1449+0856, a Cluster at z=2
• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62
• Tidal Interactions and Mergers in Intermediate Redshift EDisCS Clusters
• The Kinematics of Cluster Galaxies via Velocity Dispersion Profiles
• Characterization of Omega-WINGS galaxy clusters. I. Stellar light and mass profiles
• {\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at $z\le 0.5$
• The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• The CIDA-UCM-Yale Shallow Survey for Emission Line Galaxies
• Star formation activity of intermediate redshift cluster galaxies out to the infall regions
• Compact groups in theory and practice - II. Comparing the observed and predicted nature of galaxies in compact groups
• Galaxies in group and field environments: a comparison of optical-NIR luminosities and colors
• Morphology-dependent trends of galaxy age with environment in Abell 901/902 seen with COMBO-17
• Seyfert galaxies in UZC-Compact Groups
• Galaxy Evolution in the Environment of ABCG 209
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• Imprints of Environment on Cluster and Field Late-type Galaxies at z~1
• A Complete Spectroscopic Census of Abell 2029: A Tale of Three Histories
• The Fastest Galaxy Evolution in an Unbiased Compact Group Sample with WISE
• Measuring BAO and non-Gaussianity via QSO clustering
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• Early-Type Galaxy Star Formation Histories in Different Environments
• HiZELS: the High Redshift Emission Line Survey with UKIRT
• Photometric studies of Abell 1664: The subtle effect a minor merger has on cluster galaxies
• The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts
• Galaxy interactions in filaments and sheets: effects of the large-scale structures versus the local density
• Spatially Resolved Galaxy Star Formation and its Environmental Dependence II. Effect of the Morphology-Density Relation
• Reconstructing the galaxy density field with photometric redshifts: II. Environment-dependent galaxy evolution since $z\simeq 3$
• Star-formation rates of cluster galaxies: nature vs nurture
• The local environmental dependence of galaxy properties in the volume-limited sample of Main Galaxies from the SDSS Data Release 5
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• Dust accretion and destruction in galaxy groups and clusters
• The Ursa Major cluster redefined as a `supergroup'
• The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups
• Early-type dwarf galaxies with multicomponent stellar structure: Are they remnants of disc galaxies strongly transformed by their environment?
• SITELLE Hα Imaging Spectroscopy of z~0.25 Clusters: Emission Line Galaxy Detection and Ionized Gas Offset in Abell 2390 & Abell 2465
• Evolution of Galaxy Types and HI Gas Contents in Galaxy Groups
• Green valley galaxies in the cosmic web: internal versus environmental quenching
• Tracing the kinematics of the whole ram pressure stripped tails in ESO 137-001
• The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771
• Which halos host Herschel-ATLAS galaxies in the local Universe?
• Galaxy evolution in nearby galaxy groups. III. A GALEX view of NGC 5846, the largest group in the local universe
• Environments of dwarf galaxies with optical AGN characteristics
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Environmental impacts on dust temperature of star-forming galaxies in the local Universe
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1<z<0.35
• The effect of the environment on the structure, morphology and star-formation history of intermediate-redshift galaxies
• Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
• The puzzle of isolated and quenched dwarf galaxies in cosmic voids
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XI. Two dimensional H$\alpha$ kinematics of the edge-on ram pressure stripped galaxy NGC 4330
• Diagnostic diagrams for ram-pressure stripped candidates
• ERO R1 in CL0939+4713 field - Evidence for an S0-like galaxy at z \sim 1.5
• Spatially Resolved Spectroscopy of Passive Spiral Galaxies
• The colour-magnitude relations of ClJ1226.9+3332, a massive cluster of galaxies at z=0.89
• Environments of red nuggets at z~0.7 from the VIPERS survey
• The Evaporation and Survival of Cluster Galaxies' Coronae Part I: The Effectiveness of Isotropic Thermal Conduction Including Saturation
• Cosmic dance in the Shapley Concentration Core - I. A study of the radio emission of the BCGs and tailed radio galaxies
• Choirs, HI Galaxy Groups: Catalogue and Detection of Star-forming Dwarf Group Members
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• A Tale of Two Clusters: An Analysis of Gas-Phase Metallicity and Nebular Gas Conditions in Proto-cluster Galaxies at z~2
• The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching
• More connected, more active: galaxy clusters and groups at z~1 and the connection between their quiescent galaxy fractions and large-scale environments
• Disentangling the role of environmental processes in galaxy clusters
• Star Formation Density and Halpha Luminosity Function of an Emission Line Selected Galaxy Sample at z ~ 0.24
• The Properties of Type Ia Supernova Host Galaxies from the Sloan Digital Sky Survey
• Pre-processing of Galaxies in the Early Stages of Cluster Formation in Abell 1882 at $z$=0.139
• Segregation effects in DEEP2 galaxy groups
• The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s
• A Search for Young Stars in the S0 Galaxies of a Super-Group at z=0.37
• The Atomic Hydrogen Content of Galaxies as a function of Group-Centric Radius
• On the origin of red spirals: Does assembly bias play a role?
• On the influence of environment on star forming galaxies
• The Science Case for PILOT II: the Distant Universe
• On the Environmental Dependence of Galaxy Properties Established by the Initial Cosmological Conditions
• Star forming galaxies in the Hercules cluster: Halpha imaging of A2151
• Smaller stellar disc scale lengths in rich environments
• Linking the Structural Properties of Galaxies and their Star Formation Histories with STAGES
• Kinematics of dwarf galaxies in gas-rich groups, and the survival and detectability of tidal dwarf galaxies
• The MeerKAT Galaxy Clusters Legacy Survey: star formation in massive clusters at 0.15 < z < 0.35
• The UV window on counter rotating ETGs: insight from SPH simulations with chemo-photometric implementation
• The First Integral Field Unit Spectroscopic View of Shocked Cluster Galaxies
• Star formation rates and chemical abundances of emission line galaxies in intermediate-redshift clusters
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Optical properties of the NGC 5328 group of galaxies
• XMM-Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies
• Small-scale systems of galaxies. II. Properties of the NGC 4756 group of galaxies
• VST-GAME: Galaxy Assembly as a function of Mass and Environment with VST. Photometric assessment and density field of MACSJ0416
• CALSAGOS: Clustering ALgorithmS Applied to Galaxies in Overdense Systems
• Environmental cluster effects and galaxy evolution: The HI properties of the Abell clusters A85/A496/A2670
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
• The Origin of Star Formation in Early-type Galaxies Inferred from Spatially Resolved Spectroscopy
• The LAMOST Complete Spectroscopic Survey of Pointing Area (LaCoSSPAr) in the Southern Galactic Cap I. The Spectroscopic Redshift Catalog
• Star Formation in CALIFA survey perturbed galaxies. I. Effects of Tidal Interactions
• Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
• Properties of Galaxies in the Disc Central Surface Brightness Gap
• Signatures of Galaxy-Cluster Interactions: Tully-Fisher Observations at z~0.1
• Color, spectral and morphological transformations of galaxies in clusters
• Dorado and its member galaxies. Ha imaging of the group backbone
• The correlations between galaxy properties in different environments of the cosmic web
• A galaxy populations study of a radio-selected protocluster at z~3.1
• Star-forming galaxies in low-redshift clusters: Comparison of integrated properties of cluster and field galaxies
• Red sequence modal colour gradients across intermediate X-ray luminosity galaxy clusters
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Deep spectroscopy of nearby galaxy clusters: IV The quench of the star formation in galaxies in the infall region of Abell\ 85
• Secular evolution versus hierarchical merging: galaxy evolution along the Hubble sequence, in the field and rich environments
• Herschel and ALMA Observations of Massive SZE-selected Clusters
• Environmental effects on galaxy evolution. II: quantifying the tidal features in NIR-images of the cluster Abell 85
• A composite K-band Luminosity Function for Cluster Galaxies
• Gas properties as a function of environment in the proto-supercluster Hyperion at z ~ 2.45
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts
• Galaxy Groups: Proceedings from a Swinburne University Workshop
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• The Galaxy Population of Abell 1367: The Stellar Mass-Metallicity Relation
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• The Star Formation Rate-Density Relationship at Redshift Three
• The Rotational Profiles of Cluster Galaxies
• The effects of environment on galaxies' dynamical structures: From simulations to observations
• Comparing IMF-sensitive indices of intermediate-mass quiescent galaxies in various environments
• Interactions of galaxies outside clusters and massive groups
• Structural and dynamical modeling of WINGS clusters. III. The pseudo phase-space density profile
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters
• What size halos do local LIRGs live in?
• Environmental processing of galaxies in HI-rich groups
• No Evidence of Quasar-Mode Feedback in a Four-Way Group Merger at z~0.84
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• Environmental Effects in the Evolution of Galactic Bulges
• The XMM-SERVS X-ray eXtended Galaxy Cluster (XVXGC) catalog
• The Interplay of Cluster and Galaxy Evolution
• Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region
• A Search for Spectral Galaxy Pairs of Overlapping Galaxies based on Fuzzy Recognition
• The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours
• SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Blueberry and Green Pea galaxies live in low density environments
• Isolated and group environment dependence of stellar mass and different star formation rates
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• Main sequence of star formation and colour bimodality considering galaxy environment
• Emission line galaxies in clusters
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Star-formation Properties of z ~ 1 Galaxy Clusters and Groups from Horizon Run 5
• The evolution of cluster dwarfs
• Ecology of galaxy stellar populations from optical spectroscopic surveys
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Colour Dependence of the Distribution of IRAS Galaxies revealed by Multifractal Measures
• The History of Galaxy Formation in Groups: An Observational Perspective
• Starburst galaxies in the Hydra I cluster
• Virgo Filaments VI: H$\alpha$ clumps in the filaments around the Virgo galaxy cluster
• 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
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• The impact of encounters on the members of Local Group Analogs. A view from GALEX
• Comparison of some properties of star forming galaxies and active galactic nuclei (AGNs) between two BOSS galaxy samples of SDSS DR9