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<ri:Resource created="2022-06-03T06:34:41Z" 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>HST UV/optical photometry in NGC 1978</title><shortName>J/ApJ/906/133</shortName><identifier>ivo://CDS.VizieR/J/ApJ/906/133</identifier><altIdentifier>doi:10.26093/cds/vizier.19060133</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li C.</name></creator><creator><name>Tang B.</name></creator><creator><name>Milone A.P.</name></creator><creator><name>de Grijs R.</name></creator><creator><name>Hong J.</name></creator><creator><name>Yang Y.</name></creator><creator><name>Wang Y.</name></creator><date role="Updated">2022-09-30T22:24:51Z</date><date role="Created">2022-06-03T06:34:41Z</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>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>dwarf-stars</subject><subject>hst-photometry</subject><description>Multiple stellar populations (MPs) with different chemical compositions are not exclusive features of old globular clusters (older than 10Gyr). Indeed, recent studies reveal that younger clusters (~2-6Gyr-old) in the Magellanic Clouds also exhibit star-to-star chemical variations among evolved stars. However, whether MPs are present among less-evolved dwarfs of these intermediate-age clusters is still unclear. In this work, we search for chemical variations among GK-type dwarfs in the ~2Gyr old cluster NGC1978, which is the youngest cluster with MPs. We exploit deep ultraviolet and visual observations from the Hubble Space Telescope to constrain the nitrogen (N) and oxygen (O) variations among main-sequence (MS) stars. To do this, we compare appropriate photometric diagrams that are sensitive to N and O with synthetic diagrams of simple stellar populations and MPs. We conclude that the G- and K-type MS stars in NGC 1978 host MPs. Our statistical analysis shows that the fraction of N-rich stars ranges from ~40% to ~80%, depending on the detailed distributions of N and O.</description><source format="bibcode">2021ApJ...906..133L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/906/133</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/MNRAS/403/996">J/MNRAS/403/996 : Clusters and associations in SMC and LMC (Bonatto+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/676">J/MNRAS/430/676 : Massive clusters in the LMC (Baumgardt+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/607/A135">J/A+A/607/A135 : NGC104, 6121 &amp; 6809 AGB &amp; RGB stars Na abund. (Wang+, 2017)</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/906/133</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/906/133</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/906/133</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/906/133</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/906/133</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/906/133</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/906/133/fig2 (C_F275W,F343N,F438W_ vs. F814W diagram of NGC 1978)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/906/133/fig2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/906/133/fig2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/906/133/fig2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>82.14632</ra><dec>-66.24604</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/33113</spatial><spectral>2.0401237512456292e-19 2.706461185444514e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/906/133?format=ascii</footprint><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/906/133/fig2</name><description>C_F275W,F343N,F438W_ vs. F814W diagram of NGC 1978</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>RAJ2000</name><description>[82.1/82.3] Right Ascension, decimal degree (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>[-66.3/-66.2] Declination, decimal degree (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>F275W</name><description>[16.2/35.7] F275W UVIS-CENTER/WFC3 Vega mag (1)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F343N</name><description>[16.3/31.2] F343N UVIS-CENTER/WFC3 Vega mag (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F438W</name><description>[17.1/27.8] F438W UVIS-CENTER/WFC3 Vega mag (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814W</name><description>[15.9/25.1] F814W UVIS-CENTER/WFC3 Vega mag (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DColo</name><description>[-0.13/0.29] Color variation correction (2)</description><unit>mag</unit><ucd>phot.color;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>