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<ri:Resource created="2006-01-11T06:10:42Z" 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>Radial velocities of M49 globular clusters</title><shortName>J/ApJ/591/850</shortName><identifier>ivo://CDS.VizieR/J/ApJ/591/850</identifier><altIdentifier>doi:10.26093/cds/vizier.15910850</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cote P.</name></creator><creator><name>McLaughlin D.E.</name></creator><creator><name>Cohen J.G.</name></creator><creator><name>Blakeslee J.P.</name></creator><date role="Updated">2006-01-11T05:12:52Z</date><date role="Created">2006-01-11T06:10:42Z</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>globular-star-clusters</subject><subject>radial-velocity</subject><description>Using the Low Resolution Imaging Spectrometer on the Keck I and II telescopes, we have measured radial velocities for 196 globular clusters (GCs) around M49 (NGC 4472), the brightest member of the Virgo Cluster. Combined with published data, they bring the total number of GCs with measured radial velocities in this galaxy to 263. In terms of sample size, spatial coverage, velocity precision, and the availability of metallicity estimates from Washington photometry, this radial velocity database resembles that presented recently for M87 (NGC 4486), Virgo's cD galaxy and its second-ranked member. 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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>Class</name><description>Object classification (1)</description><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>[GLK96]</name><description>Object identification (2)</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000) (2)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000) (2)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Rad</name><description>Distance from the center of M49 (3)</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>Position angle in degrees East of North (3)</description><unit>deg</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>T1mag</name><description>The T_1_ band magnitude</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>C-T1</name><description>The (C-T_1_) color index</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>? 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