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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3275
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dc.contributor.authorReddy, B. E-
dc.contributor.authorParthasarathy, M-
dc.contributor.authorGonzalez, G-
dc.contributor.authorBakker, E. J-
dc.date.accessioned2008-08-28T14:11:01Z-
dc.date.available2008-08-28T14:11:01Z-
dc.date.issued1997-
dc.identifier.citationIAU Symposium, No. 180, p. 366en
dc.identifier.issn0074 - 1809-
dc.identifier.urihttp://hdl.handle.net/2248/3275-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997IAUS..180..366Ren
dc.subjectIRAS 05341+0852en
dc.subject21 MU M Emissionen
dc.titleThe chemical composition of IRAS 05341+0852: a post-AGB F supergiant with 21 MU M emissionen
dc.typeArticleen
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