The predicted infrared spectrum of ZrO and its possible presence in S stars

dc.contributor.author	Murty, P. S
dc.date.accessioned	2008-12-15T12:25:15Z
dc.date.available	2008-12-15T12:25:15Z
dc.date.issued	1980-04
dc.identifier.citation	Astrophysics and Space Science, Vol. 68, No. 2, pp. 513 - 518	en
dc.identifier.issn	0004-640X (Print) 1572-946X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/4059
dc.description	Open Access
dc.description.abstract	The unidentified absorption feature at 9730 Â± 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 accentuated	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Company	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1980Ap%26SS..68..513M	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00639718	en
dc.rights	D. Reidel Publishing Company
dc.subject	Astronomical Spectroscopy	en
dc.subject	Infrared Spectra	en
dc.subject	Red Giant Stars	en
dc.subject	Stellar Spectra	en
dc.subject	Zirconium Oxides	en
dc.subject	Absorption Spectra	en
dc.subject	Electron States	en
dc.subject	Electron Transitions	en
dc.subject	Franck-Condon Principle	en
dc.title	The predicted infrared spectrum of ZrO and its possible presence in S stars	en
dc.type	Article	en