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<ri:Resource created="2017-10-23T10:33:25Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Double-component model fitting of elliptical gal.</title><shortName>J/ApJ/836/115</shortName><identifier>ivo://CDS.VizieR/J/ApJ/836/115</identifier><altIdentifier>doi:10.26093/cds/vizier.18360115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Oh S.</name></creator><creator><name>Greene J.E.</name></creator><creator><name>Lackner C.N.</name></creator><date role="Updated">2020-01-29T13:59:18Z</date><date role="Created">2017-10-23T10:33:25Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>redshifted</subject><subject>galaxy-classification-systems</subject><subject>astronomical-models</subject><description>We investigate two-dimensional image decomposition of nearby, morphologically selected early-type galaxies (ETGs). We are motivated by recent observational evidence of significant size growth of quiescent galaxies and theoretical development advocating a two-phase formation scenario for ETGs. We find that a significant fraction of nearby ETGs show changes in isophotal shape that require multi-component models. The characteristic sizes of the inner and outer component are ~3 and ~15kpc. The inner component lies on the mass-size relation of ETGs at z~0.25-0.75, while the outer component tends to be more elliptical and hints at a stochastic buildup process. We find real physical differences between single- and double-component ETGs, with double-component galaxies being younger and more metal-rich. The fraction of double-component ETGs increases with increasing {sigma} and decreases in denser environments. We hypothesize that double-component systems were able to accrete gas and small galaxies until later times, boosting their central densities, building up their outer parts, and lowering their typical central ages. In contrast, the oldest galaxies, perhaps due to residing in richer environments, have no remaining hints of their last accretion episode.</description><source format="bibcode">2017ApJ...836..115O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/836/115</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/101/1561">J/AJ/101/1561 : Isophotometry of ellipticals in Abell clusters (Porter+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/142/1">J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/330/547">J/MNRAS/330/547 : Local galaxy ages and metallicities (Terlevich+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/216">J/ApJS/182/216 : Surface photometry of Virgo ellipticals (Kormendy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/427">J/ApJS/186/427 : Detailed morphology of SDSS galaxies (Nair+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/723">J/ApJ/720/723 : Compact galaxies in the local universe (Taylor+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/739/L44">J/ApJ/739/L44 : Structural data for gal. between 0.2&lt;z&lt;2.7 (Damjanov+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/888">J/MNRAS/414/888 : ATLAS3D project. III. (Emsellem+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/24">J/ApJS/203/24 : Structural parameters of gal. in CANDELS (van der Wel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/106">J/ApJ/775/106 : CANDELS passive and massive early-type gal. (Cassata+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/39">J/ApJ/793/39 : Spectrosc. properties of BOSS compact gal. 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