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<ri:Resource created="2008-11-18T20:59:25Z" 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>Iron in hot DA white dwarfs</title><shortName>J/ApJ/652/1554</shortName><identifier>ivo://CDS.VizieR/J/ApJ/652/1554</identifier><altIdentifier>doi:10.26093/cds/vizier.16521554</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vennes S.</name></creator><creator><name>Chayer P.</name></creator><creator><name>Dupuis J.</name></creator><creator><name>Lanz T.</name></creator><date role="Updated">2017-12-15T10:55:36Z</date><date role="Created">2008-11-18T20:59:25Z</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>white-dwarf-stars</subject><subject>effective-temperature</subject><subject>x-ray-sources</subject><subject>ultraviolet-astronomy</subject><description>We present a study of the iron abundance pattern in hot, hydrogen-rich (DA) white dwarfs. The study is based on new and archival far-ultraviolet spectroscopy of a sample of white dwarfs in the temperature range 30000K&lt;=Teff&lt;=64000K. 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