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<ri:Resource created="2016-01-14T15:09:22Z" 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>SDSS-DR8 isolated low-mass galaxies</title><shortName>J/ApJ/809/146</shortName><identifier>ivo://CDS.VizieR/J/ApJ/809/146</identifier><altIdentifier>doi:10.26093/cds/vizier.18090146</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bradford J.D.</name></creator><creator><name>Geha M.C.</name></creator><creator><name>Blanton M.R.</name></creator><date role="Updated">2017-12-22T05:32:29Z</date><date role="Created">2016-01-14T15:09:22Z</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>spectroscopy</subject><subject>h-i-line-emission</subject><subject>interstellar-medium</subject><subject>stellar-masses</subject><description>We study the baryon content of low-mass galaxies selected from the Sloan Digital Sky Survey (SDSS DR8), focusing on galaxies in isolated environments where the complicating physics of galaxy-galaxy interactions are minimized. We measure neutral hydrogen (HI) gas masses and line widths for 148 isolated galaxies with stellar mass between 10^7^ and 10^9.5^M_{sun}_. We compare isolated low-mass galaxies to more massive galaxies and galaxies in denser environments by remeasuring HI emission lines from the Arecibo Legacy Fast ALFA survey 40% data release. All isolated low-mass galaxies either have large atomic gas fractions or large atomic gas fractions cannot be ruled out via their upper limits. We measure a median atomic gas fraction of f_gas_=0.81+/-0.13 for our isolated low-mass sample with no systems below 0.30. At all stellar masses, the correlations between galaxy radius, baryonic mass, and velocity width are not significantly affected by environment. Finally, we estimate a median baryon to total dynamical mass fraction of f_baryon,disk_=0.15+/-0.17. We also estimate two different median baryon to halo mass fractions using the results of semi-analytic models (f_baryon,disk_=0.04+/-0.06) and abundance matching (f_baryon,halo_=0.04+/-0.02). Baryon fractions estimated directly using HI observations appear independent of environment and maximum circular velocity, while baryon fractions estimated using abundance matching show a significant depletion of baryons at low maximum circular velocities.</description><source format="bibcode">2015ApJ...809..146B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/809/146</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/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/77">VIII/77 : HI spectral properties of galaxies (Springob+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/198">VII/198 : Mark III Catalog of Galaxy Peculiar Velocities (Willick+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/220/3">J/ApJS/220/3 : SDSS-DR7 isolated galaxy morphologies (Khim+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/134">J/AJ/147/134 : Tully-Fisher relation for S^4^G galaxies (Zaritsky+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A94">J/A+A/564/A94 : CIG sample 3-D environment (Argudo-Fernandez+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A9">J/A+A/560/A9 : AMIGA. 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