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The role of radiative transfer theory in visibility modeling: Efficient approximate techniques

✍ Scribed by Ronald G. Isaacs

Book ID
113121250
Publisher
Elsevier Science
Year
1981
Tongue
English
Weight
895 KB
Volume
15
Category
Article
ISSN
0004-6981

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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