Radiative Transfer Models of Dust Shells Around Post-AGB Stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2761

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DC Field	Value	Language
dc.contributor.author	Surendiranath, R	-
dc.contributor.author	Parthasarathy, M	-
dc.contributor.author	Varghese, B. A	-
dc.date.accessioned	2008-07-21T09:43:07Z	-
dc.date.available	2008-07-21T09:43:07Z	-
dc.date.issued	2002-09	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 281, No. 4, pp. 751 – 759	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/2761	-
dc.description	Restricted Access	en
dc.description.abstract	We present a radiative transfer analysis of circumstellar dust shells around the Post-AGB stars HD 179821, HD 56126, HD 101584 and early R star HD 100764, using the code DUSTY. Parameters like mass-loss, shell inner radius, dust temperature, outflow velocity etc., are derived for HD 179821 and HD 56126 whose observed SED could be reproduced by our models.	en
dc.format.extent	93850 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/ulyx5g4316buj99n/	en
dc.subject	Radiative Transfer Analysis	en
dc.subject	Dust Shells	en
dc.subject	HD 179821	en
dc.subject	HD 56126	en
dc.subject	HD 101584	en
dc.title	Radiative Transfer Models of Dust Shells Around Post-AGB Stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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