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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4608
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dc.contributor.authorMurty, P. S-
dc.date.accessioned2009-07-02T11:01:34Z-
dc.date.available2009-07-02T11:01:34Z-
dc.date.issued1983-
dc.identifier.citationAstrophysical Letters, Vol. 23, No. 2, pp. 77 - 80en
dc.identifier.issn0004-6388-
dc.identifier.urihttp://hdl.handle.net/2248/4608-
dc.descriptionOpen Access-
dc.description.abstractSpectrograms in the 6040-7300 A wavelength region of the S star Pi Gruis reveal the presence of new molecular features attributable to CeO. Measures of band heads compared reasonably well with the laboratory spectrum. The proposed identifications are supported by the recent high resolution spectral studies of CeO in R Gem and R And. A discussion based on the identified molecular features is included on the classification of Pi Gruis as a pure S-type star.en
dc.language.isoenen
dc.publisherGordon and Beach, Science Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1983ApL....23...77Men
dc.subjectCerium Oxidesen
dc.subjectMolecular Spectraen
dc.subjectSpectral Bandsen
dc.subjectStellar Atmospheresen
dc.subjectStellar Spectraen
dc.subjectAbsorption Spectraen
dc.subjectImage Tubesen
dc.subjectSpectrum Analysisen
dc.subjectVisible Spectrumen
dc.titleIdentification of new CeO features in the S star Pi Gruisen
dc.typeArticleen
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