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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2267
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dc.contributor.authorGiridhar, S-
dc.contributor.authorArellano Ferro, A-
dc.contributor.authorMathias, P-
dc.date.accessioned2008-05-07T09:30:54Z-
dc.date.available2008-05-07T09:30:54Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 289 - 293en
dc.identifier.urihttp://hdl.handle.net/2248/2267-
dc.description.abstractOur abundance analysis of this post-AGB candidate star confirms that the HD 172481 is indeed a post-AGB star. It belongs to an important, but relatively rare class of post-AGB stars showing Li I features in their spectra. The strength of OI triplet at 7774 Å confirms its high luminosity (log, (L/L?) ~ 4). It is moderately metal-poor with [Fe/H] of - 0.6 but shows significant enrichment of s-process elements indicating that the star has gone through the third dredge-up. We find C/O of ~ 0.4 for this star. Hot Bottom Burning scenario can explain the production of Li as well as the destruction of carbon via CN cycle that could prevent C/O ratio from exceeding one.en
dc.format.extent361423 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..289Gen
dc.subjectLi-richen
dc.subjectAGB staren
dc.subjectHD 172481en
dc.titleA Li-rich post-AGB star HD 172481en
dc.typeArticleen
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