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<ri:Resource created="2023-01-18T12:06:28Z" 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>Oscillator strength ref. for Indus_0 &amp; Indus_13</title><shortName>J/ApJ/915/103</shortName><identifier>ivo://CDS.VizieR/J/ApJ/915/103</identifier><altIdentifier>doi:10.26093/cds/vizier.19150103</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hansen T.T.</name></creator><creator><name>Ji A.P.</name></creator><creator><name>Da Costa G.S.</name></creator><creator><name>Li T.S.</name></creator><creator><name>Casey A.R.</name></creator><creator><name>Pace A.B.,Cullinane L.R.</name></creator><creator><name>Erkal D.</name></creator><creator><name>Koposov S.E.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Lewis G.F.</name></creator><creator><name>Mackey D.,Simpson J.D.</name></creator><creator><name>Shipp N.</name></creator><creator><name>Zucker D.B.</name></creator><creator><name>Bland-Hawthorn J.</name></creator><creator><name>S5 Collaboration</name></creator><date role="Updated">2023-01-24T14:11:01Z</date><date role="Created">2023-01-18T12:06:28Z</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>atomic-physics</subject><subject>astronomical-reference-materials</subject><subject>stellar-associations</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>The recently discovered Indus stellar stream exhibits a diverse chemical signature compared to what is found for most other streams due to the abundances of two outlier stars, Indus_0 and Indus_13. Indus_13 exhibits an extreme enhancement in rapid neutron-capture (r-)process elements with [Eu/Fe]=+1.81. It thus provides direct evidence of the accreted nature of r-process-enhanced stars. In this paper we present a detailed chemical analysis of the neutron-capture elements in Indus_13, revealing the star to be slightly actinide poor. The other outlier, Indus_0, displays a globular cluster-like signature with high N, Na, and Al abundances, while the rest of the Indus stars show abundances compatible with a dwarf galaxy origin. Hence, Indus_0 provides the first chemical evidence of a fully disrupted dwarf containing a globular cluster. We use the chemical signature of the Indus stars to discuss the nature of the stream progenitor which was likely a chemically evolved system, with a mass somewhere in the range from Ursa Minor to Fornax.</description><source format="bibcode">2021ApJ...915..103H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/915/103</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/371">II/371 : The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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