Optical-Near Infrared Color Gradients And Merging History Of Elliptical Galaxies
arXiv:1302.3003 · doi:10.1088/0004-637X/766/2/109
Abstract
It has been suggested that merging plays an important role in the formation and the evolution of elliptical galaxies(EGs). In order to understand the past merging history of EGs, we studied the optical-NIR color gradients of 204 EGs. The use of the optical and the NIR data provides large wavelength baselines, and breaks the age-metallicity(Z) degeneracy, allowing us to derive age and Z gradients. The use of the deep SDSS Stripe 82 images make it possible for us to examine how the color/age/Z gradients are related to merging features. We find that the optical-NIR color and the age/Z gradients of EGs with tidal features are consistent with those of relaxed EGs suggesting that the two populations underwent a similar merging history on average and that mixing of stars was more or less completed before the tidal features disappear. EGs with dust features have steeper color gradients than the other two types, even after masking out dust features during the analysis, which can be due to a process involving wet merging. More importantly, we find that the scatter in the color/age/Z gradients of the relaxed and merging feature types, decreases as their luminosities increase at M > 10^{11.4} M_{\odot} but stays to be large at lower luminosities. Mean Z gradients appear nearly constant over the explored mass range, but a possible flattening is observed at the massive end. According to our toy model that predicts how the distribution of Z gradients changes as a result of major dry merging, the mean Z gradient should flatten by 40% and its scatter become smaller by 80% per a mass doubling scale if EGs evolve only through major dry merger. Our result, although limited by a number statistics at the massive end, is consistent with the picture that major dry merging is an important mechanism for the evolution for EGs at M > 10^{11.4} M_{\odot}, but less important at the lower mass range.
42 pages, 27 figures, 5 tables. Accepted for publication in ApJ
References in corpus (10)
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- Dissipation and Extra Light in Galactic Nuclei: II. 'Cusp' Ellipticals
- Spatially resolved spectroscopy of early-type galaxies over a range in mass
- The redshift evolution of early-type galaxies in COSMOS: Do massive early-type galaxies form by dry mergers?
- EzGal: A Flexible Interface for Stellar Population Synthesis Models
- Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at
- The Nature of Blue Early-Type Galaxies in the Goods Fields
- Potential of colors for determining age and metallicity of stellar populations
- The Mid-Infrared Fundamental Plane of Early-Type Galaxies
- Observed versus modelled u,g,r,i,z-band photometry of local galaxies - Evaluation of model performance
Cited by in corpus (20)
- The X-ray counterpart to the gravitational wave event GW 170817
- The Atlas3D project -- XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images
- The Progenitors of Local Ultra-massive Galaxies Across Cosmic Time: from Dusty Star-bursting to Quiescent Stellar Populations
- Correlation between Galaxy Mergers and Luminous AGN
- Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
- Massive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies
- Colors of Ellipticals from GALEX to Spitzer
- Testing the Modern Merger Hypothesis via the Assembly of Massive Blue Elliptical Galaxies in the Local Universe
- Frequency of Tidal Features Correlates with Age and Internal Structure of Early-type Galaxies
- Morphological evolution of cluster red sequence galaxies in the past 9 Gyr
- Galaxy And Mass Assembly (GAMA): Galaxy colour gradients versus colour, structure and luminosity
- Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
- Dependence of the Fundamental Plane of Early-type Galaxies on Age and Internal Structure
- SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sample
- GECKO Optical Follow-up Observation of Three Binary Black Hole Merger Events: GW190408_181802, GW190412, and GW190503_185404
- Studying the metallicity gradient in Virgo Ellipticals with E-ELT photometry of resolved stars
- Multi-wavelength structure analysis of local cluster galaxies. The WINGS project
- Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
- Analysis of the spatially-resolved -3.6m colors and dust extinction in 257 nearby NGC and IC galaxies
- Applying galactic archeology to massive galaxies using deep imaging surveys