Galaxy Luminosity Function of Dynamically Young Abell 119 Cluster: Probing the Cluster Assembly
arXiv:1603.01556 · doi:10.3847/0004-637X/822/2/92
Abstract
We present the galaxy luminosity function (LF) of the Abell 119 cluster down to mag based on deep images in the -, -, and -bands taken by using MOSAIC II CCD mounted on the Blanco 4m telescope at the CTIO. The cluster membership was accurately determined based on the radial velocity information as well as on the color-magnitude relation for bright galaxies and the scaling relation for faint galaxies. The overall LF exhibits a bimodal behavior with a distinct dip at mag ( mag), which is more appropriately described by a two-component function. The shape of the LF strongly depends on the cluster-centric distance and on the local galaxy density. The LF of galaxies in the outer, low-density region exhibits a steeper slope and more prominent dip compared with that of counterparts in the inner, high-density region. We found evidence for a substructure in the projected galaxy distribution in which several overdense regions in the Abell 119 cluster appear to be closely associated with the surrounding, possible filamentary structure. The combined LF of the overdense regions exhibits a two-component function with a distinct dip, while the LF of the central region is well described by a single Schechter function. We suggest that, in the context of the hierarchical cluster formation scenario, the observed overdense regions are the relics of galaxy groups, retaining their two-component LFs with a dip, which acquired their shapes through galaxy merging process in group environments, before they fall into a cluster.
arXiv comment18 pages, 13 figures, accepted for publication in ApJ
References in corpus (97)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Galaxy Harassment and the Evolution of Clusters of Galaxies
- The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
- How Filaments are Woven into the Cosmic Web
- The Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
- Environmental Effects on Late-Type Galaxies in Nearby Clusters
- Morphological Transformation from Galaxy Harassment
- Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
- A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes
- A New Method For Galaxy Cluster Detection I: The Algorithm
- Galaxy Zoo: the dependence of morphology and colour on environment
- The Average Mass-to-Light Profile of Galaxy Clusters
- HST photometry of dwarf elliptical galaxies in Coma, and an explanation for the alleged structural dichotomy between dwarf and bright elliptical galaxies
- The Properties of Poor Groups of Galaxies: I. Spectroscopic Survey and Results
- A ROSAT study of the cores of clusters of galaxies - I. Cooling flows in an X-ray flux-limited sample
- The properties and luminosity function of extremely low luminosity galaxies
- The 2dF Galaxy Redshift Survey: Galaxy luminosity functions per spectral type
- The accretion of galaxies into groups and clusters
- The environmental history of group and cluster galaxies in a LambdaCDM Universe
- Inclination- and dust-corrected galaxy parameters: Bulge-to-disc ratios and size-luminosity relations
- Detecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS
- The Observational Distribution of Internal Velocity Dispersions in Nearby Galaxy Clusters
- Pre-Processing of Galaxies before Entering a Cluster
- CAIRNS: The Cluster And Infall Region Nearby Survey I. Redshifts and Mass Profiles
- The origin of dwarf ellipticals in the Virgo cluster
- Inter-cluster filaments in a CDM Universe
- The DEEP2 Galaxy Redshift Survey: Evolution of the Color-Density Relation at 0.4 < z < 1.35
- The Build-up of the Colour-Magnitude Relation as a Function of Environment
- The faint end of the galaxy luminosity function
- Merging history as a function of halo environment
- The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies
- Dynamical Evolution of Galaxies in Clusters
- Ongoing Assembly of Massive Galaxies by Major Merging in Large Groups and Clusters from the SDSS
- The Assembly of Galaxy Clusters
- The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution
- WINGS-SPE Spectroscopy in the WIde-field Nearby Galaxy-cluster Survey
- Group-cluster merging and the formation of starburst galaxies
- The Different Physical Mechanisms that Drive the Star-Formation Histories of Giant and Dwarf Galaxies
- Interactions of Galaxies in the Galaxy Cluster Environment
- The 2dF Galaxy Redshift Survey: the local E+A galaxy population
- The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). I: The UV luminosity function of the central 12 sq.deg
- The IMACS Cluster Building Survey: II. Spectral Evolution of Galaxies in the Epoch of Cluster Assembly
- An H alpha Survey of 8 Abell Clusters: the dependence of tidally-induced star formation on cluster density
- The build-up of the Coma cluster by infalling substructures
- Substructure: Clues to the Formation of Clusters of Galaxies
- The Mass Assembly of Fossil Groups of Galaxies in the Millennium Simulation
- Spectroscopic Determination of the Faint End of the Luminosity Function in the Nearby Galaxy Clusters A2199 and Virgo
- The mass assembly of galaxy groups and the evolution of the magnitude gap
- The NGC 5846 Group: Dynamics and the Luminosity Function to M_R=-12
- On the lifetime of merger features of equal-mass disk mergers
- Cool core remnants in galaxy clusters
- Substructures in WINGS clusters
- Alignments of Galaxy Group Shapes with Large Scale Structure
- 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 luminosity function of the fossil group RX J1552.2+2013
- Faint dwarf spheroidals in the Fornax Cluster: A flat luminosity function
- The XMM Cluster Survey: The Stellar Mass Assembly of Fossil Galaxies
- 15 colour photometry of Landolt SA95 standard star field
- Galactic Bulges from HST NICMOS Observations: Global Scaling Relations
- The Group Evolution Multiwavelength Study (GEMS): bimodal luminosity functions in galaxy groups
- The early-type dwarf galaxy population of the Fornax cluster
- The Surface Brightness and Colour-Magnitude Relations for Fornax Cluster Galaxies
- A Spectro-photometric Search for Galaxy Clusters in SDSS
- Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at
- The red-sequence of 72 WINGS local galaxy clusters
- Star formation in galaxies along the Pisces-Cetus Supercluster filaments
- Galaxy Orbits for Galaxy Clusters in Sloan Digital Sky Survey and 2dF Galaxy Redshift Survey
- Shapley Optical Survey. I: Luminosity Functions in the Supercluster Environment
- Imprints of mass accretion on properties of galaxy clusters
- The Luminosity Functions of the Galaxy Cluster MS1054-0321 at z=0.83 based on ACS Photometry
- The orbital velocity anisotropy of cluster galaxies: evolution
- Recent Arrival of Faint Cluster Galaxies on the Red-sequence: Luminosity Functions from 119 square degrees of CFHTLS
- Spatial variations of the optical galaxy luminosity functions and red sequences in the Coma cluster: clues to its assembly history
- Deep spectroscopic luminosity function of Abell 85: no evidence for a steep upturn of the faint-end slope
- Mass-to-Light Ratios of Groups and Clusters of Galaxies
- The Early-type Dwarf-to-Giant Ratio and Substructure in the Coma Cluster
- Individual and Group Galaxies in CNOC1 clusters
- Merger relics of cluster galaxies
- Optical Luminosity Functions of the Abell Galaxy Cluster ABCG 209 at z=0.21
- The dwarf galaxy population in Abell 2218
- Keck/LRIS Spectroscopic Confirmation of Coma Cluster Dwarf Galaxy Membership Assignments
- Luminosity segregation in three clusters of galaxies (A119, 2443, 2218)
- The Galaxy Luminosity Functions down to M_R=-10 in the Coma Cluster
- The faint-end of the galaxy luminosity function in groups
- Evolution of the galaxy luminosity function in progenitors of fossil groups
- The Dynamical Origin of Early-Type Dwarfs in Galaxy Clusters: A Theoretical Investigation
- Environmental effects on the bright end of the galaxy luminosity function in galaxy clusters
- K-band luminosity (mass) segregation in AC118 at z=0.31
- The Group Evolution Multiwavelength Study (GEMS): The near-infrared luminosity function of nearby galaxy groups
- Large-Field Multicolor Study of Abell 168 : Subclusters, Dynamics and Luminosity Functions
- The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
- Alignments of the Galaxies in and around the Virgo Cluster with the Local Velocity Shear
- The faint end of the galaxy luminosity function in Abell 1689: a steep red faint end upturn at
- Multicolor Photometry Study of the Galaxy Cluster A2589: Dynamics, Luminosity Function and Star Formation History
- Local u'g'r'i'z' Standard Stars in the Chandra Deep Field-South
- Multicolor Photometry of the Galaxies in Abell 1775: Substructures, Luminosity Functions, and Star-Formation Properties
- Multicolor Photometry of the Nearby Galaxy Cluster A119
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- Dwarf Galaxy Discoveries from the KMTNet Supernova Program I. The NGC 2784 Galaxy Group
- Globular Clusters, Ultracompact Dwarfs, and Dwarf Galaxies in Abell 2744 at the Redshift of 0.308
- The SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
- Deep spectroscopy of nearby galaxy clusters: II. The Hercules cluster
- The K-band luminosity functions of cluster galaxies
- Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at
- Early-type galaxies in the Antlia Cluster: global properties
- The -band luminosity function of the rich cluster VC04 in the Vela supercluster
- Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data