Radiative Transfer Models of Dust Shells Around Post-AGB Stars

Details Radiative Transfer Models of Dust Shells Around Post-AGB Stars Radiative Transfer Models of Dust Shells Around Post-AGB Stars

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..751s&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 4, p. 751-759 (2002).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

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.

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