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Radiative transport in circumstellar dust shells

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/154233· OSTI ID:7194973
A calculation of a nongray, extended spherical circumstellar dust shell is presented. The study has been limited to an exploration of the following parameters: angular dependence of the incident field, density distribution, opacities, relative extension of the dust shell, and distance of the inner radius of the shell from the stellar surface. Anisotropic scattering has been included in an approximate manner. The results are applied to VY CMa. The properties of the model which give the best fit are a dust mixture of 70 percent iron and 30 percent silicates, an inner (outer) shell radius of 5.505 x 10/sup 14/ (3.0 x 10/sup 16/) cm, and a density law of the form n=n/sub 0/(r/R)/sup -1/. (AIP)
Research Organization:
Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz
OSTI ID:
7194973
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 204:3; ISSN ASJOA
Country of Publication:
United States
Language:
English