Radiative Transfer Models of Dust Shells Around Post-AGB Stars

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