Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5679
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dc.contributor.authorSri Ramachandran, P-
dc.contributor.authorRajamanickam, N-
dc.contributor.authorBagare, S. P-
dc.date.accessioned2012-01-27T13:53:16Z-
dc.date.available2012-01-27T13:53:16Z-
dc.date.issued2006-06-
dc.identifier.citationSerbian Astronomical Journal, No. 172, pp. 13-16en
dc.identifier.urihttp://hdl.handle.net/2248/5679-
dc.description.abstractThe Franck-Condon factors and r-centroids which are very closely related to transition probabilities, have been evaluated by the more reliable numerical integration procedure for the band systems B^{2}sum - X^{2}sum, C^{2}sum -X^{2}sum and F^{2}sum - X^{2}sum of astrophysical molecules strontium monohydride and strontium deuteride using an adequate potential. The Franck-Condon factors are more intense, particularly for the Δ ν = 0 bands, for all the systems examined here. Thus the bands of the molecules are expected to be present in sunspot spectra, SC-stars, cool M-giant stars and other prominent astrophysical sources.en
dc.language.isoenen
dc.publisherAstronomical Observatory, Serbiaen
dc.relation.urihttp://dx.doi.org/10.2298/SAJ0672013Ren
dc.rights© Astronomical Observatoryen
dc.subjectMolecular dataen
dc.subjectMethods: numericalen
dc.subjectSun: abundancesen
dc.titleEvaluation of Astrophysically Useful Parameters for Strontium Monohydride and Deuterideen
dc.typeArticleen
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