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<ri:Resource created="2005-06-17T16:13:25Z" status="active" updated="2025-05-19T09:50:00Z" 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>Draco 119 and HD 88609 equivalent widths</title><shortName>J/ApJ/612/447</shortName><identifier>ivo://CDS.VizieR/J/ApJ/612/447</identifier><altIdentifier>doi:10.26093/cds/vizier.16120447</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fulbright J.P.</name></creator><creator><name>Rich R.M.</name></creator><creator><name>Castro S.</name></creator><date role="Updated">2005-06-17T16:14:44Z</date><date role="Created">2005-06-17T16:13:25Z</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>line-intensities</subject><subject>chemically-peculiar-stars</subject><description>We report the abundance analysis of new high signal-to-noise ratio (S/N) spectra of the most metal-poor ([Fe/H]=-2.95) star currently known to be a member of a dwarf galaxy, the Draco dSph red giant D119. No absorption lines for elements heavier than Ni are detected in two Keck HIRES spectra covering the 3850-6655{AA} wavelength range, a phenomenon not previously noted in any other metal-poor star. We present upper limits for several heavy-element abundances. The most stringent limits, based on the nondetection of SrII and BaII lines, indicate that the total s- and r-process enrichment of D119 is at least 100times smaller than Galactic stars of similar metallicity. The light-element abundances are consistent with the star having formed out of material enriched primarily by massive Type II supernovae (M&gt;20-25M_{Sun}_). If this is the case, we are forced to conclude that massive, metal-poor Type II supernovae did not contribute to the r-process in the proto-Draco environment. We compare the abundance pattern observed in D119 to current predictions of prompt enrichment and pair-instability supernovae and find that the model predictions fail by an order of magnitude or more for many elements.</description><source format="bibcode">2004ApJ...612..447F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/612/447</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/612/447</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/612/447</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/612/447</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/612/447</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/612/447</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/612/447</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><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/612/447/table1</name><description>Line list</description><column><name>n_EW1</name><description>[abc] Note on EW1 (3)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n_EW2</name><description>[abc] Note on EW2 (3)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_EW1</name><description>Limit on EW1</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EW1</name><description>? Equivalent width for Draco 119</description><unit>pm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><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>lambda</name><description>Wavelength</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ion</name><description>Ion (1)</description><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>EP</name><description>Excitation potential</description><unit>eV</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>? Log of oscillator strength</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_log(gf)</name><description>[b] Flag on log(gf) (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EW2</name><description>? Equivalent width for HD88609</description><unit>pm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>