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<ri:Resource created="2015-03-05T08:46:10Z" 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>Spectroscopic HK' index for 3 globular clusters</title><shortName>J/ApJS/216/19</shortName><identifier>ivo://CDS.VizieR/J/ApJS/216/19</identifier><altIdentifier>doi:10.26093/cds/vizier.22160019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lim D.</name></creator><creator><name>Han S.-I.</name></creator><creator><name>Lee Y.-W.</name></creator><creator><name>Roh D.-G.</name></creator><creator><name>Sohn Y.-J.</name></creator><creator><name>Chun S.-H.</name></creator><creator><name>Lee J.-W.,Johnson C.I.</name></creator><date role="Updated">2015-03-30T17:59:50Z</date><date role="Created">2015-03-05T08:46:10Z</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>chemical-abundances</subject><subject>spectroscopy</subject><description>There is increasing evidence for the presence of multiple red giant branches (RGBs) in the color-magnitude diagrams of massive globular clusters (GCs). In order to investigate the origin of this split on the RGB, we have performed new narrow-band Ca photometry and low-resolution spectroscopy for M22, NGC 1851, and NGC 288. We find significant differences (more than 4{sigma}) in calcium abundance from the spectroscopic HK' index for M22 and NGC 1851. We also find more than 8{sigma} differences in CN-band strength between the Ca-strong and Ca-weak subpopulations for these GCs. For NGC 288, however, a large difference is detected only in the CN strength. The calcium abundances of RGB stars in this GC are identical to within the errors. This is consistent with the conclusion from our new Ca photometry where the RGB splits are confirmed in M22 and NGC 1851, but not in NGC 288. We also find interesting differences in the CN-CH correlations among these GCs. While CN and CH are anti-correlated in NGC 288, they show a positive correlation in M22. NGC 1851, however, shows no difference in CH between the two groups of stars with different CN strengths. We suggest that all of these systematic differences would be best explained by how strongly Type II supernovae enrichment has contributed to the chemical evolution of these GCs.</description><source format="bibcode">2015ApJS..216...19L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/216/19</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/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A13">J/A+A/563/A13 : Horizontal branch stars in M22 (Gratton+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A101">J/A+A/559/A101 : NGC6656 spectroscopy of 71 blue HB stars (Salgado+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/541/A15">J/A+A/541/A15 : Abundances of M22 subgiants (Marino+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A19">J/A+A/539/A19 : Horizontal branch stars in NGC 1851 (Gratton+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/126">J/AJ/142/126 : CN &amp; CH in SDSS Galactic globular clusters (Smolinski+, 2011)</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/ApJ/742/37">J/ApJ/742/37 : Abundances of six RGB stars in M22 (Roederer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/524/A44">J/A+A/524/A44 : CN and CH line strengths in 12 globulars (Pancino+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/839">J/MNRAS/405/839 : Spectroscopic obs. of globular clusters (Sharina+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1481">J/ApJ/705/1481 : Spectro. of stars in 6 globular clusters (Da Costa+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/437">J/A+A/486/437 : CN and CH line strengths in 8 Galactic GC (Kayser+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/637">J/ApJS/99/637 : Equivalent widths for 54 red giants (Norris+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/107/32">J/PASP/107/32 : uvby-hk photometry in M22 (Anthony-Twarog+ 1995)</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/ApJS/216/19</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/216/19</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/216/19</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/216/19</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/216/19</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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