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<ri:Resource created="2009-03-07T22:45:27Z" 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>SiS line list</title><shortName>J/ApJ/690/L122</shortName><identifier>ivo://CDS.VizieR/J/ApJ/690/L122</identifier><altIdentifier>doi:10.26093/cds/vizier.16909122</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cami J.</name></creator><creator><name>Sloan G.C.</name></creator><creator><name>Markwick-Kemper A.J.</name></creator><creator><name>Zijlstra A.A.,Bauschlicher C.W. Jr</name></creator><creator><name>Matsuura M.</name></creator><creator><name>Decin L.</name></creator><creator><name>Hony S.</name></creator><date role="Updated">2009-03-07T21:50:10Z</date><date role="Created">2009-03-07T22:45:27Z</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>atomic-physics</subject><description>We present Spitzer spectra of S stars, which are cool evolved stars with a C/O ratio near unity, some of which have enhanced s-process abundances. We present the detection of a strong and unusual band in the mid-infrared, at 13um, within the N-band window. Using quantum-chemically calculated line lists, and model spectra, we identify this band as the fundamental rovibrational band of SiS. Detection of the overtone band at 6.7um confirms the identification Fitting the line profile shows that the molecule is located in relatively cool layers, at T~1500K. We discuss these results in the context of chemical equilibrium models. The observed strength of these bands in the cool S stars makes them a promising observational diagnostic tool for studying the atmospheres of brown dwarfs and exoplanets.</description><source format="bibcode">2009ApJ...690L.122C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/690/L122</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/ApJ/690/L122</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/690/L122</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/690/L122</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/690/L122</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/690/L122</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/690/L122</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"/></coverage><tableset><schema><name>default</name><table><name>J/ApJ/690/L122/sis</name><description>SiS line list</description><column><name>E</name><description>Lower state energy</description><unit>cm**-1</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><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>sigma</name><description>Transition frequency</description><unit>cm**-1</unit><ucd>em.freq;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>A</name><description>Einstein transition probability (A-value)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>vl</name><description>Lower state vibrational quantum number</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>vu</name><description>Upper state vibrational quantum number</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Jl</name><description>Lower state angular momentum quantum number</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ju</name><description>Upper state angular momentum quantum number</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>