Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2078
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dc.contributor.authorDixit, G-
dc.contributor.authorSahoo, B. K-
dc.contributor.authorDeshmukh, P. C-
dc.contributor.authorChaudhuri, R. K-
dc.contributor.authorMajumder, S-
dc.date.accessioned2008-02-28T08:53:28Z-
dc.date.available2008-02-28T08:53:28Z-
dc.date.issued2007-10-
dc.identifier.citationThe Astrophysical Journal Supplement Series, Vol. 172, pp. 645 – 648en
dc.identifier.urihttp://hdl.handle.net/2248/2078-
dc.description.abstractAccurate ab initio calculations have been carried out to study the valence electron removal energies and oscillator strengths of astrophysically important electromagnetic transitions of quadruply ionized vanadium, V4+. Many important electron correlations are considered to all orders using the relativistic coupled-cluster theory. Calculated ionization potentials and fine-structure splittings are compared with the experimental values, wherever available. To our knowledge, oscillator strengths of electric dipole transitions are predicted for the first time for most of the transitions. The transitions span in the range of ultraviolet, visible, and near-infrared regions and are important for astrophysical observationsen
dc.format.extent101819 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherUniversity of Chicago Pressen
dc.relation.urihttp://arxiv.org/abs/physics/0702066en
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/519217en
dc.subjectatomic dataen
dc.subjectcircumstellar matteren
dc.subjectISM: atomsen
dc.titleAccurate Estimates of Circumstellar and Interstellar Lines of Quadruply Ionized Vanadium Using the Coupled Cluster Approachen
dc.typeArticleen
Appears in Collections:IIAP Publications

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