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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1465
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dc.contributor.authorAnandaraj, R-
dc.contributor.authorSankaralingam, T-
dc.contributor.authorAsokarajan, R-
dc.contributor.authorRajamanickam, N-
dc.date.accessioned2007-03-22T05:18:24Z-
dc.date.available2007-03-22T05:18:24Z-
dc.date.issued1992-
dc.identifier.citationBASI, Vol. 20, pp. 279-282en
dc.identifier.urihttp://hdl.handle.net/2248/1465-
dc.description.abstractThe 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.extent274083 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectInterstellar matteren
dc.titleAstrophysical molecule S2 - Vibrational transition probability dataen
dc.typeArticleen
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