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<ri:Resource created="2023-02-13T13:26:28Z" 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>Stellar disc scale lengths in rich environments</title><shortName>J/MNRAS/489/2216</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/489/2216</identifier><altIdentifier>doi:10.26093/cds/vizier.74892216</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Demers M.L.</name></creator><creator><name>Parker L.C.</name></creator><creator><name>Roberts I.D.</name></creator><date role="Updated">2024-08-20T20:12:47Z</date><date role="Created">2023-02-13T13:26:28Z</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>catalogs</subject><subject>x-ray-sources</subject><subject>astrometry</subject><subject>visible-astronomy</subject><description>We investigate the dependence of stellar disc scale lengths on environment for a sample of Sloan Digital Sky Survey Data Release 7 galaxies with published photometric bulge-disc decompositions. We compare disc scale lengths at fixed bulge mass for galaxies in an isolated field environment to galaxies in X-ray rich and X-ray poor groups. At low bulge mass, stellar disc scale lengths in X-ray rich groups are smaller compared to discs in both X-ray poor groups and in isolated field environments. This decrease in disc scale length is largely independent of halo mass, though shows some dependence on group-centric distance. We also find that stellar disc scale lengths are smaller in X-ray rich environments for a subset of star-forming galaxies and for galaxies of different morphological types. We note that disc scale lengths of low mass galaxies are known to have large systematic uncertainties, however we focus on differences between samples with the same measurement biases. Our results show that stellar disc scale lengths depend on X-ray brightness, a tracer of IGM density, suggesting a role for hydrodynamic processes such as ram-pressure stripping and/or starvation.</description><source format="bibcode">2019MNRAS.489.2216D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/489/2216</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/II/294">II/294 : The SDSS Photometric Catalog, Release 7</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/196/11">J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies 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(2014MNRAS.439..611W, J/MNRAS/439/611)</description><unit>1e+37W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Group</name><description>Group identifier (G3)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R/R200</name><description>Group-centric radius</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sloan</name><description>Display the online SDSS data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/489/2216/table2</name><description>data for galaxies from the XRW group sample</description><column><name>logMbulge</name><description>Logarithm of bulge mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFR</name><description>Logarithm of star formation rate from Brinchmann et al. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>SDSS object identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMstar</name><description>Logarithm of stellar mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMdisk</name><description>Logarithm of disk mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Scale</name><description>Physical scale at redshift z (G2)</description><unit>kpc/arcsec</unit><ucd>instr.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BTr</name><description>r-band bulge fraction</description><ucd>phot.mag.sb;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nb</name><description>Sersic index (G2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rd</name><description>Exponential disk scale length (G2)</description><unit>kpc</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Re</name><description>Bulge semimajor effective radius (G2)</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmax</name><description>Galaxy volume correction (G2)</description><unit>Mpc**3</unit><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PpS</name><description>F-test probability that a B+D model is not required compared to a pure Sersic model (G2)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMhalo</name><description>Logarithm of halo mass (G3)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lx</name><description>Group X-ray luminosity from Wang et al. (2014MNRAS.439..611W, J/MNRAS/439/611)</description><unit>1e+37W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Group</name><description>Group identifier (G3)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>zg</name><description>Redshift of the luminosity-weighted group centre (G3)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R200</name><description>Group viral radius (1)</description><unit>Mpc</unit><ucd>phys.size.radius;pos.lg</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R/R200</name><description>Group-centric radius</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sloan</name><description>Display the online SDSS data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/489/2216/table3</name><description>galaxies from the isolated field catalogue</description><column><name>Re</name><description>Bulge semimajor effective radius (G2)</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>SDSS object identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMstar</name><description>Logarithm of stellar mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMbulge</name><description>Logarithm of bulge mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMdisk</name><description>Logarithm of disk mass (G1)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Scale</name><description>Physical scale at redshift z (G2)</description><unit>kpc/arcsec</unit><ucd>instr.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BTr</name><description>r-band bulge fraction</description><ucd>phot.mag.sb;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nb</name><description>Sersic index (G2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rd</name><description>Exponential disk scale length (G2)</description><unit>kpc</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmax</name><description>Galaxy volume correction (G2)</description><unit>Mpc**3</unit><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PpS</name><description>F-test probability that a B+D model is not required compared to a pure Sersic model (G2)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Group</name><description>Group identifier (G3)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logSFR</name><description>Logarithm of star formation rate from Brinchmann et al. (2004MNRAS.351.1151B)</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sloan</name><description>Display the online SDSS data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>