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<ri:Resource created="2019-02-13T07:28:07Z" 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>Abundances of very metal-poor stars in Sagittarius</title><shortName>J/ApJ/855/83</shortName><identifier>ivo://CDS.VizieR/J/ApJ/855/83</identifier><altIdentifier>doi:10.26093/cds/vizier.18550083</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hansen C.J.</name></creator><creator><name>El-Souri M.</name></creator><creator><name>Monaco L.</name></creator><creator><name>Villanova S.</name></creator><creator><name>Bonifacio P.</name></creator><creator><name>Caffau E.,Sbordone L.</name></creator><date role="Updated">2019-02-25T14:18:44Z</date><date role="Created">2019-02-13T07:28:07Z</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>galaxies</subject><subject>spectroscopy</subject><subject>chemically-peculiar-stars</subject><subject>chemical-abundances</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><description>Sagittarius (Sgr) is a massive disrupted dwarf spheroidal galaxy in the Milky Way halo that has undergone several stripping events. Previous chemical studies were restricted mainly to a few, metal-rich ([Fe/H]&gt;~-1) stars that suggested a top-light initial mass function (IMF). Here we present the first high-resolution, very metal-poor ([Fe/H]=-1 to -3) sample of 13 giant stars in the main body of Sgr. We derive abundances of 13 elements, namely C, Ca, Co, Fe, Sr, Ba, La, Ce, Nd, Eu, Dy, Pb, and Th, that challenge the interpretation based on previous studies. Our abundances from Sgr mimic those of the metal-poor halo, and our most metal-poor star ([Fe/H]~-3) indicates a pure r-process pollution. Abundances of Sr, Pb, and Th are presented for the first time in Sgr, allowing for age determination using nuclear cosmochronology. We calculate ages of 9+/-2.5Gyr. Most of the sample stars have been enriched by a range of asymptotic giant branch (AGB) stars with masses between 1.3 and 5M_{sun}_. SgrJ190651.47-320147.23 shows a large overabundance of Pb (2.05dex) and a peculiar abundance pattern best fit by a 3M_{sun}_ AGB star. Based on star-to-star scatter and observed abundance patterns, a mixture of low- and high-mass AGB stars and supernovae (15-25M_{sun}_) is necessary to explain these patterns. The high level (0.29+/-0.05dex) of Ca indicates that massive supernovae must have existed and polluted the early ISM of Sgr before it lost its gas. This result is in contrast with a top-light IMF with no massive stars polluting Sgr.</description><source format="bibcode">2018ApJ...855...83H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/855/83</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/AJ/109/218">J/AJ/109/218 : Catalogue of globular cluster profiles (Trager+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/1841">J/AJ/120/1841 : Abundance &amp; Kinematic of Halo &amp; Disk Stars (Fulbright 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/381/500">J/A+A/381/500 : Eu abundances in F and G disk stars (Koch+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/340/304">J/MNRAS/340/304 : [X/Fe] of Galactic disc F and G dwarfs (Reddy+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/1117">J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1545">J/AJ/127/1545 : Abundance ratios of 4 stars in Pal 12 (Cohen+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/1091">J/ApJ/617/1091 : La and Eu abundances in 85 stars (Simmerer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1177">J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. 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