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Radiative transfer in atmospheres with spherical symmetry—III. The Eddington approximation

✍ Scribed by E. Simonneau


Publisher
Elsevier Science
Year
1978
Tongue
English
Weight
314 KB
Volume
20
Category
Article
ISSN
0022-4073

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## Abstract A protoplanetary disk is a quasi‐toroidal gas–dust mixture rotating around a protostar that creates a complex intensity field in the internal disk medium in which planets are believed to form. In this work we start to model an idealized disk describing the radiation intensity propagatin