Astrophysically Useful Parameters for Certain Band Systems of BeH, BeD and BeT Molecules

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5680

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DC Field	Value	Language
dc.contributor.author	Shanmugavel, R	-
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Rajamanickam, N	-
dc.date.accessioned	2012-01-27T14:02:18Z	-
dc.date.available	2012-01-27T14:02:18Z	-
dc.date.issued	2006-12	-
dc.identifier.citation	Serbian Astronomical Journal, No. 173, pp. 83-87	en
dc.identifier.uri	http://hdl.handle.net/2248/5680	-
dc.description.abstract	The vibronic (vibration-electronic) transition probability parameters such as Franck-Condon (FC) factors and r-centroids of diatomic molecular species could be useful in the identification of molecular bands and in the estimation of relative abundance of the emitted species in astrophysical sources. In this study, they have been evaluated for the electronic transitions A2Πr-X2Σ+, B2Πr-X2Σ+ and C2Σ+ - X2Σ+ systems of BeH, A2Πr - X2Σ and C2Σ+ - X2Σ+ system of BeD and A2Πr - X2Σ+ system of BeT molecules using a suitable potential.	en
dc.language.iso	en	en
dc.publisher	Astronomical Observatory, Serbia	en
dc.relation.uri	http://dx.doi.org/10.2298/SAJ0673083S	en
dc.rights	© Astronomical Observatory	en
dc.subject	Molecular data	en
dc.subject	Methods: numerical	en
dc.subject	Sun: abundances	en
dc.title	Astrophysically Useful Parameters for Certain Band Systems of BeH, BeD and BeT Molecules	en
dc.type	Article	en
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