Astrophysical molecule S2 - Vibrational transition probability data

dc.contributor.author	Anandaraj, R
dc.contributor.author	Sankaralingam, T
dc.contributor.author	Asokarajan, R
dc.contributor.author	Rajamanickam, N
dc.date.accessioned	2007-03-22T05:18:24Z
dc.date.available	2007-03-22T05:18:24Z
dc.date.issued	1992
dc.identifier.citation	BASI, Vol. 20, pp. 279-282	en
dc.identifier.uri	http://hdl.handle.net/2248/1465
dc.description.abstract	The study computes the Franck-Condon factors (vibrational transition probabilities) and r-centroids by the more reliable numerical integration procedure for the bands of C 3Sigma(u)(-) yields X 3Sigma(g)(-) and D3 Pi(u,r) yields X 3Sigma(g)(-) systems of the astrophysically significant S2 molecule using the suitable potential. The molecular constants are derived form Huber and Herzberg (1979).	en
dc.format.extent	274083 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Interstellar matter	en
dc.title	Astrophysical molecule S2 - Vibrational transition probability data	en
dc.type	Article	en