Planetary accretion from planetesimals to protoplanets is investigated using three-dimensional N-body simulations. The effect of gas drag due to solar nebula is included and realistic-sized planetesimals with a standard material density are used, with which the growth time scale of planetesimals is
β¦ LIBER β¦
Distribution of Planetesimals around a Protoplanet in the Nebula Gas
β Scribed by Hidekazu Tanaka; Shigeru Ida
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 485 KB
- Volume
- 120
- Category
- Article
- ISSN
- 0019-1035
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