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<ri:Resource created="2015-04-20T15:18:09Z" 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>Chemical abundances in a metal-poor RGB star</title><shortName>J/ApJ/775/L27</shortName><identifier>ivo://CDS.VizieR/J/ApJ/775/L27</identifier><altIdentifier>doi:10.26093/cds/vizier.17759027</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Johnson C.I.</name></creator><creator><name>McWilliam A.</name></creator><creator><name>Rich R.M.</name></creator><date role="Updated">2015-05-06T15:20:56Z</date><date role="Created">2015-04-20T15:18:09Z</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>chemical-abundances</subject><subject>giant-stars</subject><subject>chemically-peculiar-stars</subject><description>We present chemical abundances for 27 elements ranging from oxygen to erbium in the metal-poor ([Fe/H]=-1.67) bulge red giant branch star 2MASS 18174532-3353235. The results are based on equivalent width and spectrum synthesis analyses of a high-resolution (R~30000) spectrum obtained with the Magellan-MIKE spectrograph. While the light (Z&lt;~30) element abundance patterns match those of similar metallicity bulge and halo stars, the strongly enhanced heavy element abundances are more similar to "r-II" halo stars (e.g., CS 22892-052) typically found at [Fe/H]&lt;~-2.5. We find that the heaviest elements (Z&gt;=56) closely follow the scaled-solar r-process abundance pattern. We do not find evidence supporting significant s-process contributions; however, the intermediate mass elements (e.g., Y and Zr) appear to have been produced through a different process than the heaviest elements. The light and heavy element abundance patterns of 2MASS 18174532-3353235 are in good agreement with the more metal-poor r-process enhanced stars CS 22892-052 and BD +17{deg}3248. 2MASS 18174532-3353235 also shares many chemical characteristics with the similar metallicity but comparatively {alpha}-poor Ursa Minor dwarf galaxy giant COS 82. Interestingly, the Mo and Ru abundances of 2MASS 18174532-3353235 are also strongly enhanced and follow a similar trend recently found to be common in moderately metal-poor main-sequence turn-off halo stars.</description><source format="bibcode">2013ApJ...775L..27J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/775/L27</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/I/320">I/320 : SPM 4.0 Catalog (Girard+, 2011)</relatedResource><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/J/ApJ/765/157">J/ApJ/765/157 : Red giants abundances in the Galactic bulge (Johnson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/175">J/ApJ/749/175 : Abundances for stars in Plaut's window (Johnson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A54">J/A+A/530/A54 : Abundances of 650 bulge red giants (Gonzalez+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/108">J/ApJ/732/108 : Abundances of 92 giants in Plaut's window (Johnson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/724/975">J/ApJ/724/975 : Metal-poor stars heavy elements abundances (Roederer+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/1373">J/ApJ/722/1373 : {omega} Centauri giants abundances (Johnson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/80">J/ApJS/182/80 : Rare earth abundances (Sneden+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/51">J/ApJS/182/51 : Transition proba. of rare earth elements (Lawler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/1267">J/ApJ/667/1267 : CrI transition probabilities (Sobeck+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/1432">J/AJ/134/1432 : Proper motions in Plaut's window (Vieira+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/367/1329">J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sp</name><description>Species identifier (1)</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Z</name><description>[8/68] Atomic number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>[4966/7836.2] Wavelength ({AA})</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExPot</name><description>[0/5.9] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>[-9.8/0.7]? 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