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<ri:Resource created="2015-02-03T13:13:44Z" 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>UV star clusters in 4 elliptical galaxies</title><shortName>J/ApJ/770/137</shortName><identifier>ivo://CDS.VizieR/J/ApJ/770/137</identifier><altIdentifier>doi:10.26093/cds/vizier.17700137</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ford H.A.</name></creator><creator><name>Bregman J.N.</name></creator><date role="Updated">2015-02-27T07:42:33Z</date><date role="Created">2015-02-03T13:13:44Z</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>galaxies</subject><subject>ultraviolet-photometry</subject><description>Small amounts of star formation in elliptical galaxies are suggested by several results: surprisingly young ages from optical line indices, cooling X-ray gas, and mid-infrared dust emission. Such star formation has previously been difficult to directly detect, but using ultraviolet Hubble Space Telescope Wide Field Camera 3 imaging, we have identified individual young stars and star clusters in four nearby ellipticals. Ongoing star formation is detected in all galaxies, including three ellipticals that have previously exhibited potential signposts of star-forming conditions (NGC 4636, NGC 4697, and NGC 4374), as well as the typical "red and dead" NGC 3379. The current star formation in our closest targets, where we are most complete, is between 2.0 and 9.8x10^-5^M_{sun}_/yr. The star formation history was roughly constant from 0.5 to 1.5 Gyr (at (3-5)x10^-4^M_{sun}_/yr), but decreased by a factor of several in the past 0.3Gyr. Most star clusters have a mass between 10^2^ and 10^4^M_{sun}_. The specific star formation rates of ~10^-16^/yr (at the present day) or ~10^-14^/yr (when averaging over the past Gyr) imply that a fraction 10^-8^ of the stellar mass is younger than 100Myr and 10^-5^ is younger than 1Gyr, quantifying the level of frosting of recent star formation over the otherwise passive stellar population. There is no obvious correlation between either the presence or spatial distribution of postulated star formation indicators and the star formation we detect.</description><source format="bibcode">2013ApJ...770..137F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/770/137</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/137">J/ApJ/768/137 : Color-metallicity relations. IV. M84 GCs (Yoon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/116">J/ApJ/759/116 : Chemical analysis of NGC 4636 globular clusters (Park+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A115">J/A+A/544/A115 : Velocities of NGC 4636 globular clusters (Schuberth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/438/1163">J/A+A/438/1163 : Catalogue of Open Cluster Data (COCD) (Kharchenko+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/433/43">J/A+A/433/43 : C-T1 phot. of NGC 4636 GC system (Dirsch+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/2138">J/AJ/129/2138 : Centers of early-type galaxies with HST (Lauer+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/363/769">J/MNRAS/363/769 : Dynamical modelling of 4 early-type gal. (Samurovic+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/345/949">J/MNRAS/345/949 : UBRI photometry of NGC 3379 GCs (Whitlock+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/127/39">J/ApJS/127/39 : Stellar &amp; gas kinematics in early-type galaxies (Caon+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/96/269">J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)</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/770/137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/770/137</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/770/137</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/770/137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/770/137</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/770/137</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/770/137/table2 (Properties of UV-bright clusters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/770/137/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/770/137/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/770/137/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>161.92949167</ra><dec>12.58905278</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/26125 26313 27515 27773</spatial><spectral>5.4699463256110985e-19 9.254243743779334e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/770/137?format=ascii</footprint><waveband>UV</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/770/137/table2</name><description>Properties of UV-bright clusters</description><column><name>Seq</name><description>[1/271] Cluster ID number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Name</name><description>Host galaxy NCG name (3379, 4697, 4636 or 4374)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F225W</name><description>[21.9/25.6] HST/WFC3 F225W band magnitude</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F225W</name><description>[0.02/0.4] Uncertainty in F225Wmag</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F336W</name><description>[21/26.2] HST/WFC3 F336W band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F336W</name><description>Uncertainty in F336Wmag</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>col</name><description>[-2.3/1] The (F225W-F336W) color index</description><unit>mag</unit><ucd>phot.color;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_col</name><description>Uncertainty in color</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[100/30000]? 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