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<ri:Resource created="2016-10-03T07:45:46Z" 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>LHA 120-S 73 optical and NIR spectra</title><shortName>J/A+A/593/A112</shortName><identifier>ivo://CDS.VizieR/J/A+A/593/A112</identifier><altIdentifier>doi:10.26093/cds/vizier.35930112</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kraus M.</name></creator><creator><name>Cidale L.S.</name></creator><creator><name>Arias M.L.</name></creator><creator><name>Maravelias G.</name></creator><creator><name>Nickeler D.H.,Torres A.F.</name></creator><creator><name>Fernandes M.Borges</name></creator><creator><name>Aret A.</name></creator><creator><name>Cure M.</name></creator><creator><name>Vallverdu R.</name></creator><creator><name>Barba R.H.</name></creator><date role="Updated">2016-10-03T07:11:01Z</date><date role="Created">2016-10-03T07:45:46Z</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>emission-line-stars</subject><subject>supergiant-stars</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>B[e] supergiants are evolved massive stars, enshrouded in a dense wind and surrounded by a molecular and dusty disk. The mechanisms that drive phases of enhanced mass loss and mass ejections, responsible for the shaping of the circumstellar material of these objects, are still unclear. We aim to improve our knowledge on the structure and dynamics of the circumstellar disk of the Large Magellanic Cloud B[e] supergiant LHA 120-S 73. High-resolution optical and near-infrared spectroscopic data were obtained over a period of 16 and 7 yr, respectively. The spectra cover the diagnostic emission lines from [CaII] and [OI], as well as the CO bands. These features trace the disk at different distances from the star. We analyzed the kinematics of the individual emission regions by modeling their emission profiles. A low-resolution mid-infrared spectrum was obtained as well, which provides information on the composition of the dusty disk.</description><source format="bibcode">2016A&amp;A...593A.112K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/593/A112</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/593/A112</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/593/A112</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/593/A112</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/593/A112</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/593/A112</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/593/A112</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/593/A112/list</name><description>List of spectra</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Title</name><description>Title of the spectrum file</description><ucd>meta.title;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>Obs.date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Nlines</name><description>Number of lines in the spectrum file</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FileName</name><description>Name of the spectrum file</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>sp</name><description>Show the spectrum</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>