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<ri:Resource created="2007-06-23T17:09:52Z" 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>Manganese abundances in the Galactic disk</title><shortName>J/A+A/467/665</shortName><identifier>ivo://CDS.VizieR/J/A+A/467/665</identifier><altIdentifier>doi:10.26093/cds/vizier.34670665</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Feltzing S.</name></creator><creator><name>Fohlman M.</name></creator><creator><name>Bensby T.</name></creator><date role="Updated">2017-12-12T14:44:16Z</date><date role="Created">2007-06-23T17:09:52Z</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>late-type-stars</subject><subject>chemical-abundances</subject><description>Manganese is an iron-peak element and although the nucleosynthesis path that leads to its formation is fairly well understood, it remains unclear which objects, SN II and/or SN Ia, that contribute the majority of Mn to the interstellar medium. 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