On the e/sup1Σ/sup+ - d/sup1Σ/sup+ transition of TiO related to cool star spectra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4542

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DC Field	Value	Language
dc.contributor.author	Murty, P. S	-
dc.date.accessioned	2009-06-12T16:08:41Z	-
dc.date.available	2009-06-12T16:08:41Z	-
dc.date.issued	1977	-
dc.identifier.citation	Astrophysical Letters, Vol. 18, No. 4, pp. 143 - 144.	en
dc.identifier.issn	0888-6512	-
dc.identifier.uri	http://hdl.handle.net/2248/4542	-
dc.description.abstract	Based on the calculated intensity factors for the bands of the e/sup1Σ/sup + - d/sup 1 Σ/sup + transition of the TiO molecule, expected positions of unobserved bands are indicated, for use in studies of cool star spectra. The need for further laboratory investigation of the suggested.	en
dc.language.iso	en	en
dc.publisher	Gordon and Breach Science	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1977ApL....18..143M	en
dc.subject	Electron Transitions	en
dc.subject	M Stars	en
dc.subject	M Stars	en
dc.subject	Stellar Spectra	en
dc.subject	Titanium Oxides	en
dc.subject	Absorption Spectra	en
dc.subject	Franck-Condon Principle	en
dc.subject	Line Spectra	en
dc.subject	Tables (Data)	en
dc.title	On the e/sup1Σ/sup+ - d/sup1Σ/sup+ transition of TiO related to cool star spectra	en
dc.type	Article	en
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