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<ri:Resource created="2017-04-19T08:31:22Z" 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>Carbon-enhanced metal-poor (CEMP) star abundances</title><shortName>J/ApJ/833/20</shortName><identifier>ivo://CDS.VizieR/J/ApJ/833/20</identifier><altIdentifier>doi:10.26093/cds/vizier.18330020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yoon J.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Placco V.M.</name></creator><creator><name>Rasmussen K.C.</name></creator><creator><name>Carollo D.</name></creator><creator><name>He S.,Hansen T.T.</name></creator><creator><name>Roederer I.U.</name></creator><creator><name>Zeanah J.</name></creator><date role="Updated">2018-07-04T07:17:12Z</date><date role="Created">2017-04-19T08:31:22Z</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>chemically-peculiar-stars</subject><subject>carbon-stars</subject><description>We investigate anew the distribution of absolute carbon abundance, A(C)=log{epsilon}(C), for carbon-enhanced metal-poor (CEMP) stars in the halo of the Milky Way, based on high-resolution spectroscopic data for a total sample of 305 CEMP stars. The sample includes 147 CEMP-s (and CEMP-r/s) stars, 127 CEMP-no stars, and 31 CEMP stars that are unclassified, based on the currently employed [Ba/Fe] criterion. We confirm previous claims that the distribution of A(C) for CEMP stars is (at least) bimodal, with newly determined peaks centered on A(C)=7.96 (the high-C region) and A(C)=6.28 (the low-C region). A very high fraction of CEMP-s (and CEMP-r/s) stars belongs to the high-C region, while the great majority of CEMP-no stars resides in the low-C region. However, there exists complexity in the morphology of the A(C)-[Fe/H] space for the CEMP-no stars, a first indication that more than one class of first-generation stellar progenitors may be required to account for their observed abundances. The two groups of CEMP-no stars we identify exhibit clearly different locations in the A(Na)-A(C) and A(Mg)-A(C) spaces, also suggesting multiple progenitors. The clear distinction in A(C) between the CEMP-s (and CEMP-r/s) stars and the CEMP-no stars appears to be as successful, and likely more astrophysically fundamental, for the separation of these sub-classes as the previously recommended criterion based on [Ba/Fe] (and [Ba/Eu]) abundance ratios. This result opens the window for its application to present and future large-scale low- and medium-resolution spectroscopic surveys.</description><source format="bibcode">2016ApJ...833...20Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/833/20</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/J/ApJ/824/L19">J/ApJ/824/L19 : BD+44493 CEMP star equivalent widths (Roederer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/586/A158">J/A+A/586/A158 : Binary properties of CH and CEMP stars (Jorissen+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/121">J/ApJ/814/121 : CASH project. III. The CEMP star HE0414-0343 (Hollek+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/812/109">J/ApJ/812/109 : HST+Keck spectroscopy of bright CEMP-s stars (Placco+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/581/A22">J/A+A/581/A22 : 67 CEMP-s stars model analysis (Abate+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/171">J/ApJ/807/171 : SkyMapper Survey metal-poor star spectrosc. (Jacobson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A28">J/A+A/579/A28 : Abundances of 3 CEMP stars (Bonifacio+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/21">J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/136">J/AJ/147/136 : Stars of very low metal abundance. VI. 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