<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2024-04-22T07:42:02Z" 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>Abundances in M67 open cluster</title><shortName>J/AJ/166/154</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/154</identifier><altIdentifier>doi:10.26093/cds/vizier.51660154</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brady K.E.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Pilachowski C.A.</name></creator><creator><name>Afsar M.</name></creator><creator><name>Mace G.N.</name></creator><creator><name>Jaffe D.T.,Gosnell N.M.</name></creator><creator><name>Seifert R.</name></creator><date role="Updated">2024-11-06T20:17:53Z</date><date role="Created">2024-04-22T07:42:02Z</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>open-star-clusters</subject><subject>chemical-abundances</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>We report on the first detailed infrared chemical analysis of five binary members (S277, S997, S975, S1031, and S1195) in the open cluster M67 (NGC2682). These stars are located outside (bluer and/or brighter than) the main- sequence turnoff region in M67. High-resolution (R~45000) near-infrared spectra were obtained with the Immersion GRating INfrared Spectrograph (IGRINS) at the McDonald Observatory 2.7m Harlan J. Smith Telescope, providing full spectral coverage of the H and K bands. The abundances of C, Na, Mg, Al, Si, S, Ca, Fe, and Ni are measured using neutral atomic absorption lines. We detect vsini&gt;~25km/s in three of our program stars: S1031, S975, and S1195. We find our derived abundances to be in good agreement with turnoff star abundances, similar to published analyses of blue straggler stars in M67 from optical spectra. Detection of a carbon enhancement or depletion resulting from mass transfer is difficult due to the uncertainties in the carbon abundance and the relatively modest changes that may occur through red giant and asymptotic giant branch evolution.</description><source format="bibcode">2023AJ....166..154B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/154</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/85/315">J/ApJS/85/315 : F, G and K dwarf stars of the Pleiades (Soderblom+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/109/1379">J/AJ/109/1379 : Praesepe &amp; M 67 spectral standards (Allen+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/110/863">J/PASP/110/863 : A Stellar Spectral Flux Library: 1150 - 25000 A (Pickles 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/360/499">J/A+A/360/499 : Equivalent widths of 9 stars of M 67 (Tautvaisiene+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/382/899">J/A+A/382/899 : BVI photometry in M67 (Stassun+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/418/509">J/A+A/418/509 : Chandra observation of M67 (Van Den Berg+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/463/789">J/A+A/463/789 : Blue stragglers in open clusters (Ahumada+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/497/497">J/A+A/497/497 : Physical parameters from JHK flux (Gonzalez-Hernandez+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A56">J/A+A/511/A56 : Abundances of five open clusters (Pancino+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/59">J/AJ/142/59 : Chemical abundance in 10 open clusters (Jacobson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/97">J/AJ/150/97 : Radial velocities in M67. I. 1278 candidates (Geller+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/594/A43">J/A+A/594/A43 : APOGEE/Kepler sample stars abundances (Hawkins+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/585/A150">J/A+A/585/A150 : On the metallicity of open clusters. III. (Netopil+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/865/44">J/ApJ/865/44 : Abundances of evolved stars from IGRINS. I. (Afsar+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/869/9">J/ApJ/869/9 : Machine-learning investigation of open cluster M67 (Gao, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/238/29">J/ApJS/238/29 : IGRINS spectral library (Park+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A8">J/A+A/624/A8 : Evolved Galactic open clusters dynamical props (Angelo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/874/97">J/ApJ/874/97 : Chemical abundances from APOGEE. II. M67 stars (Souto+, 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/166/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/166/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/166/154</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/166/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/166/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/166/154</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/166/154/table2</name><description>Line List</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>Element</name><description>Atomic Line</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>lambda</name><description>[15094/22538] Vacuum wavelength; Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>chi</name><description>[1.89/9.83] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>[-1.52/0.86] log of statistical weight of lower energy level times oscillator strength of transition</description><ucd>stat.weight;phys.atmol.oscStrength;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_chi</name><description>[1/2] Reference for chi (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>