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<ri:Resource created="2011-05-18T08:56:57Z" 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>Evolution and yields of low-mass AGB stars</title><shortName>J/ApJ/696/797</shortName><identifier>ivo://CDS.VizieR/J/ApJ/696/797</identifier><altIdentifier>doi:10.26093/cds/vizier.16960797</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cristallo S.</name></creator><creator><name>Straniero O.</name></creator><creator><name>Gallino R.</name></creator><creator><name>Piersanti L.</name></creator><creator><name>Dominguez I.,Lederer M.T.</name></creator><date role="Updated">2018-09-29T17:38:03Z</date><date role="Created">2011-05-18T08:56:57Z</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>chemical-abundances</subject><subject>astronomical-models</subject><subject>giant-stars</subject><description>The envelope of thermally pulsing asymptotic giant branch (TP-AGB) stars undergoing periodic third dredge-up (TDU) episodes is enriched in both light and heavy elements, the ashes of a complex internal nucleosynthesis involving p, {alpha}, and n captures over hundreds of stable and unstable isotopes. In this paper, new models of low-mass AGB stars (2M_{sun}_), with metallicity ranging between Z=0.0138 (the solar one) and Z=0.0001, are presented. Main features are (1) a full nuclear network (from H to Bi) coupled to the stellar evolution code, (2) a mass loss-period-luminosity relation, based on available data for long-period variables, and (3) molecular and atomic opacities for C- and/or N-enhanced mixtures, appropriate for the chemical modifications of the envelope caused by the TDU. For each model, a detailed description of the physical and chemical evolutions is presented; moreover, we present a uniform set of yields, comprehensive of all chemical species (from hydrogen to bismuth).</description><source format="bibcode">2009ApJ...696..797C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/696/797</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/512/A10">J/A+A/512/A10 : Evolution of massive AGB stars. III. (Siess, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/837">J/ApJ/690/837 : CN and CO observations toward AGB stars (Milam+, 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/ApJ/696/797</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/696/797</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/696/797</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/696/797</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/696/797</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/696/797</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"/></coverage><tableset><schema><name>default</name><table><name>J/ApJ/696/797/table12</name><description>Final elemental surface composition of the 5 reference models at different metallicities</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>El/Rat</name><description>Element or ratio identification (2)</description><ucd>phys.atmol.element</ucd></column><column><name>Z1.38e-2</name><description>Final surface composition of Z=1.38e-2 model (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z6.0e-3</name><description>Final surface composition of Z=6.0e-3 model (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z3.0e-3</name><description>Final surface composition of Z=3.0e-3 model (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z1.0e-3</name><description>Final surface composition of Z=1.0e-3 model (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z1.0e-4</name><description>Final surface composition of Z=1.0e-4 model (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/696/797/table14</name><description>Stellar yields of the 5 reference models at different metallicities</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>A</name><description>[1/210] Isotope number</description><ucd>phys.atmol.weight</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>El</name><description>Element number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Z1.38e-2</name><description>Yield of Z=1.38e-2 model</description><unit>solMass</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z6.0e-3</name><description>Yield of Z=6.0e-3 model</description><unit>solMass</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z3.0e-3</name><description>Yield of Z=3.0e-3 model</description><unit>solMass</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z1.0e-3</name><description>Yield of Z=1.0e-3 model</description><unit>solMass</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Z1.0e-4</name><description>Yield of Z=1.0e-4 model</description><unit>solMass</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/696/797/tdu</name><description>Pulse by pulse elemental surface composition of the 5 models (tables 7--12 of paper)</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>Z</name><description>Metallicity (0.0138, 0.006, 0.003, 0.001 or 0.0001)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>El</name><description>Element identification</description><ucd>meta.id;phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>TDU1</name><description>1st Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU2</name><description>2nd Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU3</name><description>3rd Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU4</name><description>4th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU5</name><description>5th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU6</name><description>6th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU7</name><description>7th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU8</name><description>8th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU9</name><description>9th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU10</name><description>10th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU11</name><description>11th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TDU12</name><description>? 12th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU13</name><description>? 13th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU14</name><description>? 14th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU15</name><description>? 15th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU16</name><description>? 16th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU17</name><description>? 17th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TDU19</name><description>? 19th Third Dredge Up surface composition (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Fin</name><description>Final surface composition if the element</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>yield</name><description>Yields of the various isotopes of this element for this metallicity</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>