A Wide-field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z=0.4. III: Spectroscopic Signatures of Environmental Evolution in Early Type Galaxies
arXiv:astro-ph/0508092 · doi:10.1086/497024
Abstract
We report results from a panoramic spectroscopic survey of 955 objects in the field of the rich cluster Cl 0024+1654 (z~0.4), complementing the HST imaging presented in the first paper in this series. Our new spectroscopic sample includes over 200 high quality spectra of cluster members, spread across an area 10 Mpc in diameter. We examine the properties of a large sample of 104 cluster early-types as a function of cluster radius and local density, using them as sensitive tracers of the various physical processes that may be responsible for galaxy evolution. By constructing the Fundamental Plane of Cl 0024, we infer an evolution in the mean mass to light ratio of early-types equal to Δ<Log (M/L_V)> = -0.14 +- 0.02. In the cluster center, we detect a significantly increased scatter in the relationship compared to that seen in local clusters. Moreover, we observe a clear radial trend in the mass to light ratios of individual early types, with the oldest galaxies located in the cluster core. Galaxies are apparently younger at larger radius, with E+S0s in the periphery having M/L_V ratios that nearly match values seen in the field at a similar redshift. Independent spectral indicators used in combination reveal an abrupt interaction with the cluster environment which occurs near the virial radius of Cl 0024, revealed by small bursts of star formation in a population of dim early-types, as well as by enhanced Balmer absorption for a set of larger E+S0s closer to the cluster core. We construct a simple infall model used to compare the timescales and strengths of the observed interactions in this cluster. We examine the possibility that bursts of star formation are triggered when galaxies suffer shocks as they encounter the intra-cluster medium, or by the onset of galaxy harassment.
arXiv comment27 pages, 14 figures, Accepted by ApJ
References in corpus (71)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Stellar population synthesis at the resolution of 2003
- Detailed Structural Decomposition of Galaxy Images
- Galaxy Harassment and the Evolution of Clusters of Galaxies
- Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies
- Differential Galaxy Evolution in Cluster and Field Galaxies at z=0.3
- Morphological Transformation from Galaxy Harassment
- Stellar population models of Lick indices with variable element abundance ratios
- Galaxy Star-Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey
- The Star Formation Histories of Galaxies in Distant Clusters
- The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters
- Old Stellar Populations. VI. Absorption-Line Spectra of Galaxy Nuclei and Globular Clusters
- Gone with the wind: the origin of S0 galaxies in clusters
- A Spectroscopic Catalog of 10 Distant Rich Clusters of Galaxies
- The Fundamental Plane for cluster E and S0 galaxies
- Science Objectives and Early Results of the DEEP2 Redshift Survey
- Dynamical family properties and dark halo scaling relations of giant elliptical galaxies
- Cosmological Shock Waves and Their Role in the Large Scale Structure of the Universe
- On the Survival and Destruction of Spiral Galaxies in Clusters
- The Morphology - Density Relation in z ~ 1 Clusters
- A wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius
- The evolution of the galactic morphological types in clusters
- A JavaScript Passive Evolution Calculator
- The Fundamenal Plane in CL0024 at z=0.4: Implications for the Evolution of the Mass-to-Light Ratio
- The evolution of substructure III: the outskirts of clusters
- The Assembly History of Field Spheroidals: Evolution of Mass-to-light Ratios and Signatures of Recent Star Formation
- A Wide Field Hubble Space Telescope Study of the Cluster Cl0024+1654 at z=0.4 II: The Cluster Mass Distribution
- Keck Spectroscopy of distant GOODS Spheroidal Galaxies: Downsizing in a Hierarchical Universe
- Evolution Since z=1 of the Morphology-density Relation of Galaxies
- The Observational Consequences of Merging Clusters of Galaxies
- Galaxy Evolution in Abell 2390
- A comparison of the galaxy populations in the Coma and distant clusters: the evolution of k+a galaxies and the role of the intracluster medium
- Mass-to-Light Ratios of Field Early-Type Galaxies at z~1 from Ultra-Deep Spectroscopy: Evidence for Mass-dependent Evolution
- The Transformation of Galaxies within the Large Scale Structure around a z=0.41 Cluster
- On the dependence of spectroscopic indices of early-type galaxies on age, metallicity and velocity dispersion
- The evolution of field early-type galaxies to z~0.7
- A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies
- The Evolution of a Mass-Selected Sample of Early-Type Field Galaxies
- The Colour-Magnitude Relation as a Constraint on the Formation of Rich Cluster Galaxies
- The Evolution of Early-Type Galaxies in Distant Clusters III.: M/L_V Ratios in the z=0.33 Cluster CL1358+62
- H-alpha Photometry of Abell 2390
- The Properties of Field Elliptical Galaxies at Intermediate Redshift. I: Empirical Scaling Laws
- A Spectroscopic Survey of the Galaxy Cluster CL 1358+62 at z=0.328
- Exploring Cluster Ellipticals as Cosmological Standard Rods
- Clustering at High Redshift: Precise Constraints from a Deep, Wide Area Survey
- The properties of field elliptical galaxies at intermediate redshift. II: photometry and spectroscopy of an HST selected sample
- A Panoramic Halpha Imaging Survey of the z=0.4 cluster Cl0024.0+1652 with Subaru
- The properties of field elliptical galaxies at intermediate redshift. III: the Fundamental Plane and the evolution of stellar populations from z~0.4 to z=0
- A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654. II. A high-speed collision?
- The Fundamental Plane of Cluster Ellipticals at z = 1.25
- The detailed Fundamental Plane of two high redshift clusters: MS 2053-04 at z=0.58 and MS 1054-03 at z=0.83
- The Evolution of Early-Type Galaxies in Distant Clusters I.: Surface Photometry and Structural Parameters for 53 Galaxies in the z=0.33 Cluster CL1358+62
- Large-Scale Structure Shocks at Low and High Redshifts
- The Origin of the Spatial Distribution of X-ray luminous AGN in Massive Galaxy Clusters
- A new catalogue of ISM content of normal galaxies
- The Tully-Fisher relation of cluster spirals at z = 0.83
- Gas Dynamic Stripping and X-Ray Emission of Cluster Elliptical Galaxies
- Galaxy Morphologies in the Cluster CL1358+62 at z=0.33
- A wide-field spectroscopic survey of the cluster of galaxies Cl0024+1654: I. The catalogue
- The Evolution of Balmer Absorption Line Strengths in E/S0 Galaxies from z=0 to z=0.83
- Internal Color Properties of Resolved Spheroids in the Deep HST/ACS field of UGC 10214
- Measuring age, metallicity and abundance ratios from absorption line indices
- The Tully-Fisher relation of distant cluster galaxies
- The Transformation of Cluster Galaxies at Intermeidate Redshift
- The early-type galaxy population in Abell 2218
- XMM-Newton study of the lensing cluster of galaxies CL0024+17
- On the evolutionary status of early-type galaxies in clusters at z~0.2 - I. The Fundamental Plane
- Internal kinematics of spiral galaxies in distant clusters Part I
- Kinematic and chemical evolution of early-type galaxies
- RXJ0142.0+2131: I. The galaxy content of an X-ray-luminous galaxy cluster at z=0.28
- Star formation activity of intermediate redshift cluster galaxies out to the infall regions
Cited by in corpus (69)
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- The evolution of the star formation activity in galaxies and its dependence on environment
- The Sloan-Lens ACS Survey II: stellar populations and internal structure of early-type lens galaxies
- Ultraviolet Detection of the Tidal Disruption of a Star by a Supermassive Black Hole
- A Wide-field Survey of Two Z~0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s
- The Rise and Fall of Passive Disk Galaxies: Morphological Evolution Along the Red Sequence Revealed by COSMOS
- The DEEP3 Galaxy Redshift Survey: The Impact of Environment on the Size Evolution of Massive Early-type Galaxies at Intermediate Redshift
- Evolution of the Color-Magnitude Relation in Galaxy Clusters at z ~1 from the ACS Intermediate Redshift Cluster Survey
- Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17
- The relation between star formation, morphology and local density in high redshift clusters and groups
- The environments of starburst and post-starburst galaxies at z=0.4-0.8
- Galaxy evolution in overdense environments at high redshift: passive early-type galaxies in a cluster at redshift 2
- LoCuSS: The steady decline and slow quenching of star formation in cluster galaxies over the last four billion years
- The Star Formation Epoch of the Most Massive Early-Type Galaxies
- A Panoramic Mid-infrared Survey of Two Distant Clusters
- LoCuSS: The mid-infrared Butcher-Oemler effect
- The Las Campanas/AAT Rich Cluster Survey III: Spectroscopic Studies of X-ray Bright Galaxy Clusters at z~0.1
- Galaxy Assembly Bias on the Red Sequence
- Spitzer/MIPS 24um Observations of Galaxy Clusters: An Increasing Fraction of Obscured Star-forming Members from z=0.02 to z=0.83
- Cosmic Chronometers: Constraining the Equation of State of Dark Energy. II. A Spectroscopic Catalog of Red Galaxies in Galaxy Clusters
- A More Fundamental Plane
- Spectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields
- Properties of the galaxy population in hydrodynamical simulations of clusters
- Stellar populations and evolution of early-type cluster galaxies: Constraints from optical imaging and spectroscopy of z=0.5-0.9 galaxy clusters
- Photometric mass and mass decomposition in early-type lens galaxies
- The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6um, 4.5um, 5.8um and 8.0um Cluster Luminosity Functions
- The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
- Plunging fireworks: Why do infalling galaxies light up on the outskirts of clusters?
- Line Strengths in Early-Type Cluster Galaxies at z=0.33: Implications for alpha/Fe, Nitrogen and the Histories of E/S0s
- X-ray Bright Active Galactic Nuclei in Massive Galaxy Clusters II: The Fraction of Galaxies Hosting Active Nuclei
- Star formation in galaxies along the Pisces-Cetus Supercluster filaments
- Star formation in galaxies falling into clusters along supercluster-scale filaments
- Multiscale probability mapping: groups, clusters and an algorithmic search for filaments in SDSS
- Dynamical Models of Elliptical Galaxies in z=0.5 Clusters: II. Mass-to-Light Ratio Evolution without Fundamental Plane Assumptions
- Abell 851 and the Role of Starbursts in Cluster Galaxy Evolution
- The nature of dusty starburst galaxies in a rich cluster at z=0.4: the progenitors of lenticulars?
- Diffuse optical intracluster light as a measure of stellar tidal stripping: the cluster CL0024+17 at 0.4 observed at LBT
- GALEX Observations of "Passive Spirals" in the Cluster Cl 0024+17: Clues to the Formation of S0 Galaxies
- Dynamical Evidence for Environmental Evolution of Intermediate Redshift Spiral Galaxies
- LoCuSS: Probing Galaxy Transformation Physics with Herschel
- Shapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores
- Star Formation in the Bullet Cluster I: The Infrared Luminosity Function and Star Formation Rate
- X-ray bright active galactic nuclei in massive galaxy clusters III: New insights into the triggering mechanisms of cluster AGN
- The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
- Evolution of the Stellar Mass--Metallicity Relation - I: Galaxies in the z~0.4 Cluster Cl0024
- Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
- The Dynamical Distinction between Elliptical and Lenticular Galaxies in Distant Clusters: Further Evidence for the Recent Origin of S0 Galaxies
- Tracing the Peculiar Dark Matter Structure in the Galaxy Cluster CL 0024+17 with Intracluster Stars and Gas
- ACCESS III: The Nature of Star Formation in the Shapley Supercluster
- LoCuSS: Shedding New Light on the Massive Lensing Cluster Abell 1689 - The View From Herschel
- Infalling Faint [OII] Emitters in Abell 851. II. Environment, Kinematics, and Star Formation History
- Data and 2D scaling relations for galaxies in Abell 1689: a hint of size evolution at z~0.2
- Stellar populations in hosts of giant radio galaxies and their neighbouring galaxies
- GLACE survey: OSIRIS/GTC Tuneable Filter H imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue
- A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z 0.4
- The role of environment in low-level active galactic nucleus activity: no evidence for cluster enhancement
- Spitzer observations of Abell 1763 - I: infrared and optical photometry
- The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s
- The Gemini/HST Galaxy Cluster Project: Stellar Populations in the Low Redshift Reference Cluster Galaxies
- Infalling Faint [OII] Emitters in Abell 851. I. Spectroscopic Confirmation of Narrowband-Selected Objects
- A Census of Mid-Infrared Selected Active Galactic Nuclei in Massive Galaxy Clusters at 0 < z < 1.3
- Disentangling the Dynamical Mechanisms for Cluster Galaxy Evolution
- Cl 1103.7-1245 at z=0.96: the highest redshift galaxy cluster in the EDisCS survey
- Efficient detection of emission line galaxies in the Cl0016+1609 and MACSJ1621.4+3810 supercluster filaments using SITELLE
- Environmental Effects in the Evolution of Galactic Bulges
- Galaxy evolution studies in clusters: the case of Cl0024+1652 cluster galaxies at z0.4
- GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652 II. The mass--metallicity relationship and the effect of the environment
- GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
- A catalog of X-ray point sources in the Abell 133 region