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<ri:Resource created="2014-12-08T09:31:49Z" 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>Galaxy groups and clouds in the local universe</title><shortName>J/MNRAS/412/2498</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/412/2498</identifier><altIdentifier>doi:10.26093/cds/vizier.74122498</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Makarov D.</name></creator><creator><name>Karachentsev I.</name></creator><date role="Updated">2024-07-13T20:15:00Z</date><date role="Created">2014-12-08T09:31:49Z</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>galaxy-clusters</subject><description>We present an all-sky catalogue of 395 nearby galaxy groups revealed in the Local Supercluster and its surroundings. The groups and their associations are identified among 10914 galaxies at |b|&gt;15{deg} with radial velocities V_LG_&lt;3500km/s. Our group-finding algorithm requires the group members to be located inside their zero-velocity surface. Hereby, we assume that individual galaxy masses are proportional to their total K-band luminosities, M/L_K_=6M_{sun}_/L_{sun}_. The sample of our groups, where each group has n&gt;=4 members, is characterized by the following medians: mean projected radius &lt;R&gt;=268kpc, radial velocity dispersion {sigma}_V_=74km/s, K-band luminosity L_K_=1.2x10^11^L_{sun}_, virial and projected masses M_vir_=2.4x10^12^ and M_p_=3.3x10^12^M_{sun}_, respectively. Accounting for measurement error reduces the median masses by 30 per cent. For 97 per cent of identified groups the crossing time does not exceed the cosmic time, 13.7Gyr, with the median at 3.8Gyr. We examine different properties of the groups, in particular of the known nearby groups and clusters in Virgo and Fornax. About a quarter of our groups can be classified as fossil groups where the dominant galaxy is at least 10 times brighter than the other group members.</description><source format="bibcode">2011MNRAS.412.2498M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/412/2498</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/ApJ/743/123">J/ApJ/743/123 : Coma I cloud fast motions of galaxies (Karachentsev+, 2011)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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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>Group</name><description>Principal name of the group's brightest galaxy, taken, as a rule, from LEDA</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension of group's main member (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination of the group's main member (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>N</name><description>[4/355] Number of group members with known radial velocities</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VLG</name><description>Mean radial velocity of the group relative to the centroid of the Local Group</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sigV</name><description>Standard deviation of radial velocities of the group members {sigma}_V_ not corrected for the velocity measurement errors</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rh</name><description>Mean harmonic radius of the group (1)</description><unit>kpc</unit><ucd>phys.size.radius;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logLK</name><description>Total luminosity of the group in the Ks band (2)</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM</name><description>Projected mass of the group, as defined by Heisler et al. 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