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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2130
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dc.contributor.authorKarthikeyan, B-
dc.contributor.authorRaja, V-
dc.contributor.authorRajamanickam, N-
dc.contributor.authorBagare, S. P-
dc.date.accessioned2008-03-06T05:03:52Z-
dc.date.available2008-03-06T05:03:52Z-
dc.date.issued2007-12-
dc.identifier.citationSerbian Astronomical Journal, No. 175, pp. 25 - 32en
dc.identifier.urihttp://hdl.handle.net/2248/2130-
dc.descriptionOpen Access-
dc.description.abstractIn molecular astrophysics, the Franck-Condon (FC) factors and r-centroids are essential for the interpretation of spectral intensities in terms of emitting astrophysical source conditions. They have been evaluated for the band systems a 3Πr - X 1Σ+, d3Δni - X 1Σ+- X 1Σ+, e 3Σ- - X 1Σ+, A' 1Σ+ - X 1Σ+ and d3Δni and - a 3Πr of astrophysical molecule CS. The physical and astrophysical significances of our evaluated FC factors and r-centroids are discussed. The FC factor values of a - X system have been compared with the values of FC factors reported by Reddy et al. (2003).en
dc.format.extent189191 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherNational Library of Serbiaen
dc.relation.uridoi:10.2298/SAJ0775025Ken
dc.relation.urihttp://saj.matf.bg.ac.yu/175/pdf/025-032.pdfen
dc.relation.urihttp://saj.matf.bg.ac.yu/175.html#SAJ0775025Ken
dc.subjectmolecular dataen
dc.subjectmethods: numericalen
dc.subjectsun: abundancesen
dc.subjectstars: abundancesen
dc.titleOn the Franck-Condon factors and R-centroids of the astrophysically interesting molecule CSen
dc.typeArticleen
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