Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4056
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dc.contributor.authorMurty, P. S-
dc.date.accessioned2008-12-15T11:26:47Z-
dc.date.available2008-12-15T11:26:47Z-
dc.date.issued1980-08-
dc.identifier.citationAstrophysical Journal, Part 1, Vol. 240, pp. 363 - 367en
dc.identifier.urihttp://hdl.handle.net/2248/4056-
dc.descriptionOpena Access-
dc.description.abstractIn 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.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1980ApJ...240..363Men
dc.relation.urihttp://www.journals.uchicago.edu/toc/apj/current-
dc.rightsAmerican Astronomical Society-
dc.subjectStellar Spectraen
dc.subjectTransition Probabilitiesen
dc.subjectLine Identifications-
dc.subjectMolecular Processes-
dc.subjectStars-S type-
dc.titleOn the E 1 Pi-X 1 Sigma + and 1 Sigma +-X 1 Sigma + transitions of ZrO related to S star spectraen
dc.typeArticleen
Appears in Collections:IIAP Publications

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