Evaluation of astrophysically useful parameters for HD molecule

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DC Field	Value	Language
dc.contributor.author	Karthikeyan, B	-
dc.contributor.author	Rajamanickam, N	-
dc.contributor.author	Bagare, S. P	-
dc.date.accessioned	2008-09-02T14:48:48Z	-
dc.date.available	2008-09-02T14:48:48Z	-
dc.date.issued	2006-10	-
dc.identifier.citation	Astroparticle Physics, Vol. 26, No. 3, pp. 186 - 189	en
dc.identifier.issn	0927-6505	-
dc.identifier.uri	http://hdl.handle.net/2248/3337	-
dc.description	Restricted Access	en
dc.description.abstract	The spectrum of HD molecule is the testing ground of both refined calculations and experimental techniques and its excited states are of considerable relevance to chemistry and astrophysics. In this study, the Franck Condon (FC) factors and r-centroids are evaluated for the bands of d3Π a3Σg+, e 3Σu+ a3Σg+ and I 1Π B1Σu+ transitions of HD molecule. The evaluation is done by numerical integration procedure using a suitable potential. The physical and astrophysical significance of the estimated FC factors and r-centroids are also discussed.	en
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/10.1016/j.astropartphys.2006.06.002	en
dc.subject	Astrophysical Molecule HD	en
dc.subject	Franck–Condon Factors	en
dc.subject	r-Centroids	en
dc.title	Evaluation of astrophysically useful parameters for HD molecule	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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