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<ri:Resource created="2024-08-23T08:58:11Z" 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 gradient of stellar populations</title><shortName>J/A+A/688/A180</shortName><identifier>ivo://CDS.VizieR/J/A+A/688/A180</identifier><altIdentifier>doi:10.26093/cds/vizier.36880180</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Scalco M.</name></creator><creator><name>Bedin L.</name></creator><creator><name>Vesperini E.</name></creator><date role="Updated">2024-11-29T20:04:46Z</date><date role="Created">2024-08-23T08:58:11Z</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>hst-photometry</subject><subject>proper-motions</subject><description>In this paper we present the analysis of Hubble Space Telescope (HST) observations of the globular cluster Omega Centauri. Our analysis combines data obtained in this work with previously published HST data from an earlier article of this series and {encompasses} a broad portion of the cluster's radial extension. Our findings reveal a significant radial variation in the fraction of stars within the two largest stellar populations, showing that one of the main second-population groups (referred to as the blue main sequence (bMS) group) is more centrally concentrated than the first-population group (referred to as the red main sequence (rMS) group). Additionally, we explore the spatial variations of the other, smaller stellar populations (referred to as MSa and MSd) and find a qualitatively similar, but weaker, radial decrease in the fraction of stars in these populations at larger distances from the cluster centre. Only one of the populations identified (MSe) does not show any significant radial variation.</description><source format="bibcode">2024A&amp;A...688A.180S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/688/A180</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/853/86">J/ApJ/853/86 : HST large programme on {omega} Centauri. II. 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Fraction of stars obtained solely from the counts of classified stars, for the central field</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Frcs</name><description>? Fraction of stars error obtained solely from the counts of classified stars, for the central field</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Fr3</name><description>? Fraction of stars for the field F3</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fr3</name><description>? Fraction of stars error for the field F3</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Fr3s</name><description>? Fraction of stars obtained solely from the counts of classified stars, for the field F3</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fr3s</name><description>? Fraction of stars error obtained solely from the counts of classified stars, for the field F3</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NST1</name><description>? Number of stars for the field F1</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Fr1</name><description>? Fraction of stars for the field F1</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Fr5</name><description>? Fraction of stars for the field F5</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fr5</name><description>? Fraction of stars error for the field F5</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Fr5s</name><description>? Fraction of stars obtained solely from the counts of classified stars, for the field F5</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fr5s</name><description>? Fraction of stars error obtained solely from the counts of classified stars, for the field F5</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NST4</name><description>? 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Fraction of stars obtained solely from the counts of classified stars, for the field F1</description><unit>%</unit><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fr1s</name><description>? Fraction of stars error obtained solely from the counts of classified stars, for the field F1</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NST5</name><description>? 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RADXS value (3)</description><ucd>meta.code</ucd><flag>nullable</flag></column><column><name>Nf</name><description>Number of single exposures star is found</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ng</name><description>Number of good measurements</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/688/A180/gaia_id</name><description>Gaia identification number for sources in common</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>Field identifier</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ID</name><description>Star internal identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GaiaDR3</name><description>? Gaia DR3 internal identification number</description><ucd>meta.id</ucd><flag>nullable</flag></column></table><table><name>J/A+A/688/A180/b18</name><description>Bellini et al. (2018ApJ...853...86B, Cat. J/ApJ/853/86) identification number for sources in common</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>Field identifier</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ID</name><description>Star internal identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B18</name><description>? Bellini et al. (2018ApJ...853...86B, Cat. J/ApJ/853/86) internal identification number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/A+A/688/A180/pop_id</name><description>Population identifier</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>Field identifier</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>ID</name><description>Star internal identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Pop</name><description>Population identifier (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sPop</name><description>Sub-population identifier (2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>