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 |