Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4643
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dc.contributor.authorSivarani, T-
dc.contributor.authorParthasarathy, M-
dc.contributor.authorGarcía, L. P-
dc.contributor.authorManchado, A-
dc.date.accessioned2009-07-15T16:06:20Z-
dc.date.available2009-07-15T16:06:20Z-
dc.date.issued2001-08-
dc.identifier.citationSzczerba, R. and Garny, S. K., eds., Post-AGB objects as a phase of stellar evolution, Astrophysics and Space Science Library, Vol. 265, Proceedings of the Torun Workshop held July 5 - 7, 2000, pp. 305 – 308en
dc.identifier.isbn0-7923-7145-3-
dc.identifier.urihttp://hdl.handle.net/2248/4643-
dc.descriptionRestricted Access-
dc.description.abstractIRAS 10215-5916 was classified as a post-AGB star and also as a massive red supergiant. It was also found to be a spectroscopic binary. In our high resolution spectra we found molecular features from a cool star of Teff = 3750K. We also see the spectral signature of a relatively hotter star of Teff = 7250K. We found that both the components of the binary system are metal poor. From the theoretical spectrum synthesis we obtained [C/H] = -0.2 +/- 0.4, [O/H] = -1.0 +/- 0.4 and [Fe/H] = -2.0 +/- 0.5 for the hot component of the binary system. The enhanced carbon abundance and metal poor characteristics show that the hot component of the binary system could be a post-AGB star.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.ispartofseriesAstrophysics and Space Science Library; Vol. 265-
dc.relation.urihttp://adsabs.harvard.edu/abs/2001ASSL..265..305Sen
dc.subjectSpectroscopy of Post-AGBen
dc.subjectIRAS 10215-5916en
dc.titleSpectroscopy of post-AGB candidate IRAS 10215-5916en
dc.typeArticleen
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