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<ri:Resource created="2019-10-01T08:49:55Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" 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/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>Tucana dSph CMD and star formation history</title><shortName>J/A+A/630/A116</shortName><identifier>ivo://CDS.VizieR/J/A+A/630/A116</identifier><altIdentifier>doi:10.26093/cds/vizier.36300116</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Savino A.</name></creator><creator><name>Tolstoy E.</name></creator><creator><name>Salaris M.</name></creator><creator><name>Monelli M.</name></creator><creator><name>de Boer T.J.L.</name></creator><date role="Updated">2019-10-01T07:58:14Z</date><date role="Created">2019-10-01T08:49:55Z</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>stellar-ages</subject><subject>hst-photometry</subject><subject>hertzsprung-russell-diagram</subject><description>We report a new star formation history for the Tucana dwarf spheroidal galaxy, obtained from a new look at a deep HST/ACS colour-magnitude diagram. We combined information from the main sequence turn-off and the horizontal branch to resolve the ancient star formation rates on a finer temporal scale than previously possible. We show that Tucana experienced three major phases of star formation, two very close together at ancient times and the last one ending between 6 and 8 Gyr ago. We show that the three discrete clumps of stars on the horizontal branch are linked to the distinct episodes of star formation in Tucana. The spatial distribution of the clumps reveals that each generation of stars presents a higher concentration than the previous one. The simultaneous modelling of the horizontal branch and the main sequence turn-off also allows us to measure the amount of mass lost by red giant branch stars in Tucana with unprecedented precision, confirming dwarf spheroidals to be excellent laboratories to study the advanced evolution of low-mass stars.</description><source format="bibcode">2019A&amp;A...630A.116S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/630/A116</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/315/40">J/A+A/315/40 : Photometry of the Tuc dwarf galaxy (Saviane, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/1742">J/ApJ/699/1742 : LCID project. I. Cetus and Tucana variables (Bernard+, 2009)</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/A+A/630/A116</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/630/A116</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/630/A116</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/630/A116</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/630/A116</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/630/A116</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><coverage><spectral>2.0401237512456292e-19 4.9761815603361e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/630/A116/table1</name><description>Star formation history</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>[alpha/Fe]</name><description>Mean alpha enhancement of the bin</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Mean [Fe/H] of the bin</description><ucd>phys.abund.Fe;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>Mean look back time of the bin</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SFR</name><description>Star formation rate in the bin</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SFR</name><description>Uncertainty on the star formation rate</description><unit>solMass/yr</unit><ucd>stat.error;phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/630/A116/phot</name><description>HST/ACS photometry</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>F475W</name><description>Magnitude in the F475W band</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F475W</name><description>? Error on the F475W magnitude (1)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>Magnitude in the F814W band</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F814W</name><description>? Error on the F814W magnitude (1)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>