dc.contributor.author |
Murty, P. S |
|
dc.date.accessioned |
2008-12-15T11:26:47Z |
|
dc.date.available |
2008-12-15T11:26:47Z |
|
dc.date.issued |
1980-08 |
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dc.identifier.citation |
Astrophysical Journal, Part 1, Vol. 240, pp. 363 - 367 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/4056 |
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dc.description |
Opena Access |
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dc.description.abstract |
In view of the prevalent interest in the singlet band systems of ZrO, which are present in the spectra of pure S stars, values of band intensity factors (FCFs) and r-centroids are evaluated and displayed for the e1 Pi - X1 Sigma + and 1 Sigma+ - X1 Sigma + transitions. The results suggest the possible presence of new bands in both the systems and warrant a reinvestigation of the spectrum of ZrO in the 5500-6600 A region. Predicted band head positions of the new bands are presented to aid both laboratory and stellar spectral studies. |
en |
dc.language.iso |
en |
en |
dc.publisher |
American Astronomical Society |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1980ApJ...240..363M |
en |
dc.relation.uri |
http://www.journals.uchicago.edu/toc/apj/current |
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dc.rights |
American Astronomical Society |
|
dc.subject |
Stellar Spectra |
en |
dc.subject |
Transition Probabilities |
en |
dc.subject |
Line Identifications |
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dc.subject |
Molecular Processes |
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dc.subject |
Stars-S type |
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dc.title |
On the E 1 Pi-X 1 Sigma + and 1 Sigma +-X 1 Sigma + transitions of ZrO related to S star spectra |
en |
dc.type |
Article |
en |