The Environmental Dependence of the Luminosity-Size Relation for Galaxies
arXiv:1004.1107 · doi:10.1088/0004-637X/715/1/606
Abstract
We have examined the luminosity-size relationship as a function of environment for 12150 SDSS galaxies with precise visual classifications from the catalog of Nair & Abraham (2010a). Our analysis is subdivided into investigations of early-type galaxies and late-type galaxies. Early-type galaxies reveal a surprisingly tight luminosity-size relation. The dispersion in luminosity about the fiducial relation is only ~0.14 dex (0.35 mag), even though the sample contains galaxies which differ by a factor of almost 100 in luminosity. The dispersion about the luminosity-size relation is comparable to the dispersion about the fundamental plane, even though the luminosity-size relation is fundamentally simpler and computed using purely photometric parameters. The key contributors to the dispersion about the luminosity-size relation are found to be color and central concentration. Expanding our analysis to the full range of morphological types, we show that the slope, zero point, and scatter about the luminosity-size relation is independent of environmental density. Our study thus indicates that whatever process is building galaxies is doing so in a way that preserves fundamental scaling laws even as the typical luminosity of galaxies changes with environment. However, the distribution of galaxies along the luminosity-size relation is found to be strongly dependent on galaxy environment. This variation is in the sense that, at a given morphology, larger and more luminous galaxies are rarer in sparser environments. Our analysis of late-type galaxy morphologies reveals that scatter increases towards later Hubble types. Taken together, these results place strong constraints on conventional hierarchical models in which galaxies are built up in an essentially stochastic way.
20 pages, 10 figures, 5 tables, Submitted Nov 5, 2009; Accepted by ApJ April 6, 2010 Higher resolution versions of the figures can be found at: http://www.bo.astro.it/~nair/Morphology/
References in corpus (17)
- Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
- A Catalog of Detailed Visual Morphological Classifications for 14034 Galaxies in the Sloan Digital Sky Survey
- Ages and metallicities of early-type galaxies in the SDSS: new insight into the physical origin of the colour-magnitude and the Mg2-sigmaV relations
- How special are Brightest Group and Cluster Galaxies?
- The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history
- Environmental Effects on Satellite Galaxies: The Link Between Concentration, Size and Colour Profile
- Curvature in the scaling relations of early-type galaxies
- Dissecting the Red Sequence--I. Star Formation Histories of Quiescent Galaxies: The Color-Magnitude vs. the Color-Sigma Relation
- Structural Properties of Central Galaxies in Groups and Clusters
- Evolution in the structural properties of early-type Brightest Cluster Galaxies at small lookback time and dependence on the environment
- The Morphology of Passively Evolving Galaxies at z ~ 2 from HST/WFC3 Deep Imaging in the Hubble Ultradeep Field
- The importance of dry and wet merging on the formation and evolution of elliptical galaxies
- Photometric Properties and Scaling Relations of Early Type Brightest Cluster Galaxies
- The growth of luminous red galaxies by merging
- Gas Mass Fractions and Star Formation in Blue-Sequence E/S0 Galaxies
- Predicting the Properties of the Remnants of Dissipative Galaxy Mergers
- The Magnitude-Diameter Relation of Galaxies
Cited by in corpus (31)
- From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
- Spectroscopic Confirmation of the Rich z=1.80 Galaxy Cluster JKCS 041 Using the WFC3 Grism: Environmental Trends in the Ages and Structure of Quiescent Galaxies
- The DEEP3 Galaxy Redshift Survey: The Impact of Environment on the Size Evolution of Massive Early-type Galaxies at Intermediate Redshift
- Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies
- Clues from nearby galaxies to a better theory of cosmic evolution
- A Census of Oxygen in Star-Forming Galaxies: An Empirical Model Linking Metallicities, Star Formation Rates and Outflows
- Size Evolution of Spheroids in a Hierarchical Universe
- Tracing Galaxies Through Cosmic Time with Number Density Selection
- A Detection of Weak Lensing Magnification using Galaxy Sizes and Magnitudes
- The Relation Between Galaxy Morphology and Environment in the Local Universe: An RC3-SDSS Picture
- Massive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies
- The DiskMass Survey. IV. The Dark-Matter-Dominated Galaxy UGC 463
- A Detection of the Environmental Dependence of the Sizes and Stellar Haloes of Massive Central Galaxies
- The Role of Dissipation in the Scaling Relations of Cosmological Merger Remnants
- Comparing galaxy populations in compact and loose groups of galaxies
- Size distribution of galaxies in SDSS DR7: weak dependence on halo environment
- A Fundamental Line for Elliptical Galaxies
- A Comparison Between the Half-Light Radii, Luminosities, and UBV Colors of Globular Clusters in M31 and the Galaxy
- The VIMOS Public Extragalactic Redshift Survey (VIPERS) -- Environment-size relation of massive passive galaxies at 0.5 < z < 0.8
- Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
- Environments of red nuggets at z~0.7 from the VIPERS survey
- Stellar Mass Profiles of Quiescent Galaxies in Different Environments at
- Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
- Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
- Overview of the Near-IR S0 galaxy Survey (NIRS0S)
- What determines the sizes of red early-type galaxies?
- Quantifying galactic morphological transformations in the cluster environment
- Measurable Relationship Between Bright Galaxies and Their Faint Companions in WHL J085910.0+294957, a Galaxy Cluster at z = 0.30: Vestiges of Infallen Groups?
- Do Galaxies Change in Size ? An Angular Size Test at Low Redshift with SDSS Data
- Environmental Invariance of the Galaxy Size-Mass Relation
- Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour