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<ri:Resource created="2012-03-26T14:45:02Z" 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>Quadratic F_ij_ force field in l-CH_4_^-^</title><shortName>J/ApJ/708/1452</shortName><identifier>ivo://CDS.VizieR/J/ApJ/708/1452</identifier><altIdentifier>doi:10.26093/cds/vizier.17081452</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Senent M.L.</name></creator><creator><name>Hochlaf M.</name></creator><date role="Updated">2012-04-11T07:57:54Z</date><date role="Created">2012-03-26T14:45:02Z</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>Using state-of-the-art theoretical methods, we investigate the stable isomers of C^-^_4_, C_4_H and C_4_H^-^. Three of them are relevant for astrophysics and astrochemistry. These computations are performed using highly correlated ab initio methods and the aug-cc-pVXZ (X=T,Q) basis sets. In addition to the linear isomers, we predict the existence of several cyclic and branched forms for these molecules. For all the molecular species of interest here, sets of spectroscopic parameters are determined with perturbation theory, which compare quite well with experiment. For l-C_4_H^-^(X^1^{Sigma}^+^), the quartic force field is computed at the coupled cluster level of theory. This force field is derived from full nine-dimensional potential energy surface generated close to the equilibrium geometry of this anion. Finally, we treat the thermochemistry of the hydrogen attachment and the electron attachment reactions that may lead to the formation of the C_4_H^-^ from either C^-^_4_ or C_4_H.</description><source format="bibcode">2010ApJ...708.1452S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/708/1452</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/708/1452</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/708/1452</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/708/1452</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/708/1452</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/708/1452</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/708/1452</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/708/1452/table4</name><description>*(R)CCSD(T)/aug-cc-pVTZ quadratic F_ij_ force field of l-CH_4_^-^</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>i</name><description>[-7/7] The i component of the force field</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>j</name><description>[-7/7] The j component of the force field</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>k</name><description>[-7/7] The k component of the force field (1)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l</name><description>[-6/7] The l component of the force field (1)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Term</name><description>Most significant term</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>