<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2017-11-15T06:27:09Z" status="active" updated="2025-06-13T15:25:00Z" 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>Line list for the NGC 1851 stars</title><shortName>J/MNRAS/446/3319</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/446/3319</identifier><altIdentifier>doi:10.26093/cds/vizier.74463319</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yong D.</name></creator><creator><name>Grundahl F.</name></creator><creator><name>Norris J.E.</name></creator><date role="Updated">2024-08-14T20:19:04Z</date><date role="Created">2017-11-15T06:27:09Z</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>globular-star-clusters</subject><subject>apparent-magnitude</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><subject>spectroscopy</subject><description>We measure the C+N+O abundance sum in red giant stars in two Galactic globular clusters, NGC 1851 and NGC 6752. NGC 1851 has a split subgiant branch which could be due to different ages or C+N+O content while NGC 6752 is representative of the least complex globular clusters. For NGC 1851 and NGC 6752, we obtain average values of A(C+N+O)=8.16+/-0.10 ({sigma}=0.34) and 7.62+/-0.02 ({sigma}=0.06), respectively. When taking into account the measurement errors, we find a constant C+N+O abundance sum in NGC 6752. The C+N+O abundance dispersion is only 0.06 dex, and such a result requires that the source of the light element abundance variations does not increase the C+N+O sum in this cluster. For NGC 1851, we confirm a large spread in C+N+O. In this cluster, the anomalous RGB has a higher C+N+O content than the canonical RGB by a factor of 4 (~0.6 dex). This result lends further support to the idea that the two subgiant branches in NGC 1851 are roughly coeval, but with different CNO abundances.</description><source format="bibcode">2015MNRAS.446.3319Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/446/3319</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/A+A/333/479">J/A+A/333/479 : NGC 1851 dynamical and evolutionary properties</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/404/187">J/A+A/404/187 : Equivalent widths for metal-poor stars (Gratton+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A69">J/A+A/533/A69 : Spectroscopy of 124 RGB stars in NGC 1851 (Carretta+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/3044">J/MNRAS/442/3044 : Photometry and abundances of NGC1851 stars (Marino+, 2014)</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/MNRAS/446/3319</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/446/3319</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/446/3319</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/446/3319</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/446/3319</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/446/3319</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/MNRAS/446/3319/table2 (Stellar parameters and CNO abundances for NGC 1851)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/446/3319/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/446/3319/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/446/3319/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>78.4977083</ra><dec>-40.0896083</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/34242-34243</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/446/3319?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/446/3319/table2</name><description>Stellar parameters and CNO abundances for NGC 1851</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>Name</name><description>Star name (NR NNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>OName</name><description>? Other star name (NNN) (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vmag</name><description>V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CMD</name><description>Group from colour-magnitude diagram</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt</name><description>? Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_Vt</name><description>[a] Note on Vt (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Fe/H]</name><description>? Metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>C</name><description>? Carbon abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N</name><description>? Nitrogen abundance (3)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>O</name><description>? Oxygen abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>C+N+O</name><description>? Carbon nitrogen and oxygen abundance sum</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/446/3319/table4</name><description>Line list for the NGC 1851 stars</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>Lambda</name><description>Wavelength ({AA})</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Species</name><description>Species identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LEP</name><description>Lower Excitation Potential</description><unit>eV</unit><ucd>phys.atmol.excitation;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>Log of the oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Line1</name><description>? NR 712 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line2</name><description>? NR 1290 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line3</name><description>? NR 1469 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line4</name><description>? NR 2352 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line5</name><description>? NR 2953 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line6</name><description>? NR 3213 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line7</name><description>? NR 3272 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line8</name><description>? NR 4740 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line9</name><description>? NR 5171 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line10</name><description>? NR 5246 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line11</name><description>? NR 5543 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line12</name><description>? NR 6217 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line13</name><description>? NR 6221 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line14</name><description>? NR 6250 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Line15</name><description>? NR 8066 line wavelength (m{AA})</description><unit>0.1pm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Source</name><description>[ABC] Source (2)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>