Transition Probability Parameters for Certain Band Systems of the Astrophysical Molecule PO

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5678

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DC Field	Value	Language
dc.contributor.author	Balachandra Kumar, K	-
dc.contributor.author	Raja, V	-
dc.contributor.author	Nagarajan, K	-
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Rajamanickam, N	-
dc.date.accessioned	2012-01-27T13:41:13Z	-
dc.date.available	2012-01-27T13:41:13Z	-
dc.date.issued	2002	-
dc.identifier.citation	Baltic Astronomy, Vol. 11, pp. 529-535	en
dc.identifier.uri	http://hdl.handle.net/2248/5678	-
dc.description.abstract	The transition probability parameters, Franck-Condon factors and r-centroids have been evaluated by a new more reliable numerical integration procedure for the bands of the PO molecule in the ultraviolet region (1800--2900 Å). These molecules are likely to be present in the atmospheres of cool stars and comets.	en
dc.language.iso	en	en
dc.publisher	Institute of Theoretical Physics and Astronomy of Vilnius University	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BaltA..11..529B	en
dc.rights	© Institute of Theoretical Physics and Astronomy	en
dc.subject	Molecular data	en
dc.subject	Frank-Condon factors	en
dc.subject	PO molecule	en
dc.subject	stars: late-type	en
dc.title	Transition Probability Parameters for Certain Band Systems of the Astrophysical Molecule PO	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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