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 |