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<ri:Resource created="1999-01-24T16:41:44Z" 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>Central Fornax Cluster. II. Galaxy spectroscopy</title><shortName>J/A+AS/134/75</shortName><identifier>ivo://CDS.VizieR/J/A+AS/134/75</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hilker M.</name></creator><creator><name>Infante L.</name></creator><creator><name>Vieira G.</name></creator><creator><name>Infante L.</name></creator><creator><name>Kissler-Patig M.,Richtler T.</name></creator><date role="Updated">1999-01-24T15:42:11Z</date><date role="Created">1999-01-24T16:41:44Z</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>galaxy-clusters</subject><subject>radial-velocity</subject><description>In this paper, radial velocities of 94 galaxies brighter than about V_tot=20mag in the direction of the central Fornax cluster have been measured. The galaxies have been selected from the photometric catalog of Paper I (Hilker et al., 1998, Cat. &lt;J/A+AS/134/59&gt;). Most of the velocity determinations of the fainter galaxies are based on strong emission lines of late type galaxies. Table 2 of this paper contains the position, magnitude and velocity of all galaxies. Except for 8 Fornax members, all galaxies lie in the background. Among the 8 members, there are 5 nucleated dwarf ellipticals that are already listed in the FCC (Ferguson, 1989, Cat. &lt;VII/180&gt;). Two of the 3 "new" members are very compact and have surface brightnesses comparable to globular clusters, however their luminosities are in the range of dwarf elliptical nuclei.</description><source format="bibcode">1999A&amp;AS..134...75H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/134/75</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/VII/180">VII/180 : Galaxies in 3.5 degs of Fornax cluster (Fergusson+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/134/59">J/A+AS/134/59 : Paper I. 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