The chemical composition of IRAS 05341+0852: a post-AGB F supergiant with 21 MU M emission

dc.contributor.author	Reddy, B. E
dc.contributor.author	Parthasarathy, M
dc.contributor.author	Gonzalez, G
dc.contributor.author	Bakker, E. J
dc.date.accessioned	2008-08-28T14:11:01Z
dc.date.available	2008-08-28T14:11:01Z
dc.date.issued	1997
dc.identifier.citation	IAU Symposium, No. 180, p. 366	en
dc.identifier.issn	0074 - 1809
dc.identifier.uri	http://hdl.handle.net/2248/3275
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1997IAUS..180..366R	en
dc.subject	IRAS 05341+0852	en
dc.subject	21 MU M Emission	en
dc.title	The chemical composition of IRAS 05341+0852: a post-AGB F supergiant with 21 MU M emission	en
dc.type	Article	en