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<ri:Resource created="2014-01-29T12:25:54Z" 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>Spectroscopic observations in VV124 (UGC 4879)</title><shortName>J/ApJ/751/46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/751/46</identifier><altIdentifier>doi:10.26093/cds/vizier.17510046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kirby E.N.</name></creator><creator><name>Cohen J.G.</name></creator><creator><name>Bellazzini M.</name></creator><date role="Updated">2014-02-15T15:01:52Z</date><date role="Created">2014-01-29T12:25:54Z</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>radial-velocity</subject><subject>metallicity</subject><subject>line-intensities</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>VV124 (UGC 4879) is an isolated, dwarf irregular/dwarf spheroidal (dIrr/dSph) transition-type galaxy at a distance of 1.36 Mpc. Previous low-resolution spectroscopy yielded inconsistent radial velocities for different components of the galaxy, and photometry hinted at the presence of a stellar disk. In order to quantify the stellar dynamics, we observed individual red giants in VV124 with the Keck/Deep Extragalactic Imaging Multi-Object Spectrograph (DEIMOS). We validated members based on their positions in the color-magnitude diagram, radial velocities, and spectral features. Our sample contains 67 members. The average radial velocity is &lt;v_r_&gt;=-29.1+/-1.3km/s in agreement with the previous radio measurements of H I gas. The velocity distribution is Gaussian, indicating that VV124 is supported primarily by velocity dispersion inside a radius of 1.5 kpc. Outside that radius, our measurements provide only an upper limit of 8.6km/s on any rotation in the photometric disk-like feature. The velocity dispersion is {sigma}_v_=9.4+/-1.0km/s, from which we inferred a mass of M_1/2_=(2.1 +/-0.2)x10^7^M_{sun}_ and a mass-to-light ratio of (M/L_V_)_1/2_=5.2+/-1.1M_{sun}_/L_{sun}_, both measured within the half-light radius. Thus, VV124 contains dark matter. We also measured the metallicity distribution from neutral iron lines. The average metallicity, &lt;[Fe/H]&gt;=-1.14+/-0.06, is consistent with the mass-metallicity relation defined by dSph galaxies. The dynamics and metallicity distribution of VV124 appear similar to dSphs of similar stellar mass.</description><source format="bibcode">2012ApJ...751...46K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/751/46</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/J/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A37">J/A+A/533/A37 : VI HST photometry of VV124 = UGC4879 (Bellazzini+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/352">J/ApJS/191/352 : Milky Way dwarf satellites abundances (Kirby+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/328">J/ApJ/705/328 : Abundance measurements in Sculptor dSph (Kirby+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/1217">J/ApJ/682/1217 : Abundances in red giants in 7 globular clusters (Kirby+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/162">J/ApJ/659/162 : CAS parameters of 199 nearby galaxies (Taylor-Mager+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/281">J/MNRAS/380/281 : Faint galactic satellites spectro. survey (Martin+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/117/227">J/PASP/117/227 : Properties of 101 galaxies from the NFGS (Kewley+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/784">J/ApJ/630/784 : UBVR observations of nearby galaxies (Taylor+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/414/23">J/A+A/414/23 : CCD H{alpha} and R photometry of 334 galaxies (James+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/149/327">J/ApJS/149/327 : JKs photometry of local universe galaxies (Grauer+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/543/178">J/ApJ/543/178 : Nearby Optical Galaxy (NOG) sample (Giuricin+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/126/331">J/ApJS/126/331 : Spectrophotometry of nearby field galaxies (Jansen+ 2000)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/751/46</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/751/46</mirrorURL><mirrorURL 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Logarithmic iron abundance relative to the Sun</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]</name><description>[0.2/0.5]? Uncertainty in [Fe/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mm</name><description>[N/Y] Object considered to be member of VV124?</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n_Mm</name><description>Reason(s) object considered to be non-member (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>B11</name><description>Cross-match with Bellazzini et al., 2011, Cat. 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