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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4059
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dc.contributor.authorMurty, P. S-
dc.date.accessioned2008-12-15T12:25:15Z-
dc.date.available2008-12-15T12:25:15Z-
dc.date.issued1980-04-
dc.identifier.citationAstrophysics and Space Science, Vol. 68, No. 2, pp. 513 - 518en
dc.identifier.issn0004-640X (Print) 1572-946X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4059-
dc.descriptionOpen Access-
dc.description.abstractThe unidentified absorption feature at 9730 ± 5 A observed in the spectra of pure S stars is provisionally identified with the predicted 9732 A (0, 0) band of the e `IT-c `z\ transition of ZrO molecule. Relative band strengths and band head positions of this transition in the 8300- 12 500 A region are presented to assist both laboratory and stellar spectral studies. The insistent need for the laboratory study of gas phase infrared spectrum of ZrO is accentuateden
dc.language.isoenen
dc.publisherD. Reidel Publishing Companyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1980Ap%26SS..68..513Men
dc.relation.urihttp://dx.doi.org/10.1007/BF00639718en
dc.rightsD. Reidel Publishing Company-
dc.subjectAstronomical Spectroscopyen
dc.subjectInfrared Spectraen
dc.subjectRed Giant Starsen
dc.subjectStellar Spectraen
dc.subjectZirconium Oxidesen
dc.subjectAbsorption Spectraen
dc.subjectElectron Statesen
dc.subjectElectron Transitionsen
dc.subjectFranck-Condon Principleen
dc.titleThe predicted infrared spectrum of ZrO and its possible presence in S starsen
dc.typeArticleen
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