## Abstract A protoplanetary disk is a quasiβtoroidal gasβdust 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
Radiative transport in finite homogenous cylinders by the Monte Carlo technique
β Scribed by L.W. Avery; L.L. House; A. Skumanich
- Publisher
- Elsevier Science
- Year
- 1969
- Tongue
- English
- Weight
- 916 KB
- Volume
- 9
- Category
- Article
- ISSN
- 0022-4073
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