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<ri:Resource created="2021-07-28T11:25:52Z" 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>Chemical abundances in 52 M-giant stars</title><shortName>J/AJ/161/183</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/183</identifier><altIdentifier>doi:10.26093/cds/vizier.51610183</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Maas Z.G.</name></creator><creator><name>Pilachowski C.A.</name></creator><date role="Updated">2022-01-17T12:33:51Z</date><date role="Created">2021-07-28T11:25:52Z</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>milky-way-galaxy</subject><subject>giant-stars</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>We measured ^35^Cl abundances in 52-M giants with metallicities in the range -0.5&lt;[Fe/H]&lt;0.12. Abundances and atmospheric parameters were derived using infrared spectra from CSHELL on the NASA Infrared Telescope Facility and from optical echelle spectra. We measured Cl abundances by fitting a H^35^Cl molecular feature at 3.6985{mu}m with synthetic spectra. We also measured the abundances of O, Ca, Ti, and Fe using atomic absorption lines. We find that the [Cl/Fe] ratio for our stars agrees with chemical evolution models of Cl, and the [Cl/Ca] ratio is broadly consistent with the solar ratio over our metallicity range. Both indicate that Cl is primarily made in core-collapse supernovae with some contributions from Type Ia supernovae. We suggest that other potential nucleosynthesis processes, such as the {nu}-process, are not significant producers of Cl. Finally, we also find our Cl abundances are consistent with HII and planetary nebular abundances at a given oxygen abundance, although there is scatter in the data.</description><source format="bibcode">2021AJ....161..183M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/183</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/508/355">J/A+A/508/355 : Scaled solar tracks and isochrones (Bertelli+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/619">J/ApJ/711/619 : {alpha}-element abundances in galactic PNe (Milingo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/427/343">J/MNRAS/427/343 : IR excesses of Hipparcos stars (McDonald+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/78">J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A71">J/A+A/562/A71 : Chemical abund. solar neighbourhood dwarfs (Bensby+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/629/A128">J/A+A/629/A128 : Spectra of molecular absorbers (Wallstrom+, 2019)</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/AJ/161/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/161/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/161/183</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/161/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/161/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/161/183</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/AJ/161/183/table1 (and observation summary)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/161/183/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/161/183/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/161/183/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>13.3889064</ra><dec>48.5188569</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/196 2858 3203 5574 5647 8573 8762 9030 9153 9245 9435 9441 9578 9818 9838 9964 10737 10840 11594 12900 13089 14753 14765 14905 14917 14924 14952 15006 15243 22994 23422 23469 24207 26415 26423 26578 27687 28050 28649 31629 31682 31923 31990 31996 32123 32170 32190 32308 32414 32519 32652</spatial><spectral>7.952274030004205e-20 1.0188844282367877e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/161/183?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/161/183/table1</name><description>and observation summary</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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