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Evaluation of Astrophysically Useful Parameters for Strontium Monohydride and Deuteride

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dc.contributor.author Sri Ramachandran, P
dc.contributor.author Rajamanickam, N
dc.contributor.author Bagare, S. P
dc.date.accessioned 2012-01-27T13:53:16Z
dc.date.available 2012-01-27T13:53:16Z
dc.date.issued 2006-06
dc.identifier.citation Serbian Astronomical Journal, No. 172, pp. 13-16 en
dc.identifier.uri http://hdl.handle.net/2248/5679
dc.description.abstract The 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.iso en en
dc.publisher Astronomical Observatory, Serbia en
dc.relation.uri http://dx.doi.org/10.2298/SAJ0672013R en
dc.rights © Astronomical Observatory en
dc.subject Molecular data en
dc.subject Methods: numerical en
dc.subject Sun: abundances en
dc.title Evaluation of Astrophysically Useful Parameters for Strontium Monohydride and Deuteride en
dc.type Article en


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