We present numerical simulations of the interaction of a onedimensional radiative gas dynamic shock wave with a dust cloud in the solar nebula that is finite in dimension parallel to the direction of shock propagation. Energy and momentum transfer to the shock-heated gas as the gas penetrates the du
β¦ LIBER β¦
Shock wave model for the Orion KL nebula
β Scribed by Toru Okuda
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 141 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0083-6656
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