## AU), or when the secondary has a very low mass and near The accretion of planetesimals from a turbulent gas and circular orbit as in the Sun-Jupiter system. The discrepancy dust nebula is not well understood theoretically even in with the present numerical study is due in part to the different
โฆ LIBER โฆ
Computer simulation of planet formation in a binary star system: Terrestrial planets
โ Scribed by B. B. Djakov; B. I. Reznikov
- Publisher
- Springer Netherlands
- Year
- 1980
- Tongue
- English
- Weight
- 739 KB
- Volume
- 23
- Category
- Article
- ISSN
- 1573-0794
No coin nor oath required. For personal study only.
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