Accretional evolution of a planetesimal swarm: 1. A new simulation
- 31 July 1991
- Vol. 92 (1) , 147-164
- https://doi.org/10.1016/0019-1035(91)90041-q
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Accretion rates of protoplanetsIcarus, 1990
- Artificial acceleration in accumulation due to coarse mass-coordinate divisions in numerical simulationIcarus, 1990
- On collisional disruption: Experimental results and scaling lawsIcarus, 1990
- Growth of the earth in nebular gasIcarus, 1988
- From icy planetesimals to outer planets and cometsIcarus, 1984
- Collisional Processes of Planetesimals with a Protoplanet under the Gravity of the Proto-SunProgress of Theoretical Physics, 1983
- Accumulation of planetesimals in the solar nebulaIcarus, 1983
- Orbital interactions - A new geometrical formalismThe Astronomical Journal, 1982
- Planetesimals to planets: Numerical simulation of collisional evolutionIcarus, 1978
- The origin of meteorites as small bodies. II. The modelThe Astrophysical Journal, 1965