Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2760
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dc.contributor.authorMajumder, S-
dc.contributor.authorMerlitz, H-
dc.contributor.authorGopakumar, G-
dc.contributor.authorDas, B. P-
dc.contributor.authorMahapatra, U. S-
dc.contributor.authorMukherjee, Debashis-
dc.date.accessioned2008-07-21T09:36:34Z-
dc.date.available2008-07-21T09:36:34Z-
dc.date.issued2002-07-
dc.identifier.citationThe Astrophysical Journal, Vol. 574, No. 1, pp. 513 - 517en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2760-
dc.descriptionRestricted Accessen
dc.description.abstractOne of the most successful ab initio, highly correlated all-order many-body methods, the relativistic coupled cluster theory, is employed to calculate excitation energies of the doublet states of Mg+ and allowed transitions among them that are of interest in astrophysical problems. We have also calculated oscillator strength for the 3s-4p doublet transitions, which is improved over the existing results. These transition lines have been sought after in astronomical observations because they represent the best column density identifier in the interstellar medium. Our calculated oscillator strength (9.3×10-4) and branching ratio (1.80) of these doublet lines matches well with the recent empirical and semiempirical calculations.en
dc.format.extent96331 bytes-
dc.format.extent96331 bytes-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Astronomical Society.en
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/340939en
dc.subjectAtomic Dataen
dc.subjectMethods: Analyticalen
dc.titleAccurate Calculations of Interstellar Lines of Mg+ Using the Coupled Cluster Approachen
dc.typeArticleen
Appears in Collections:IIAP Publications

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