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On the Franck-Condon factors and R-centroids of the astrophysically interesting molecule CS

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dc.contributor.author Karthikeyan, B
dc.contributor.author Raja, V
dc.contributor.author Rajamanickam, N
dc.contributor.author Bagare, S. P
dc.date.accessioned 2008-03-06T05:03:52Z
dc.date.available 2008-03-06T05:03:52Z
dc.date.issued 2007-12
dc.identifier.citation Serbian Astronomical Journal, No. 175, pp. 25 - 32 en
dc.identifier.uri http://hdl.handle.net/2248/2130
dc.description Open Access
dc.description.abstract In 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.extent 189191 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher National Library of Serbia en
dc.relation.uri doi:10.2298/SAJ0775025K en
dc.relation.uri http://saj.matf.bg.ac.yu/175/pdf/025-032.pdf en
dc.relation.uri http://saj.matf.bg.ac.yu/175.html#SAJ0775025K en
dc.subject molecular data en
dc.subject methods: numerical en
dc.subject sun: abundances en
dc.subject stars: abundances en
dc.title On the Franck-Condon factors and R-centroids of the astrophysically interesting molecule CS en
dc.type Article en


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