Gaseous drag and planetary formation by accretion
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[1] G. Wetherill,et al. The range of validity of the two-body approximation in models of terrestrial planet accumulation: I. Gravitational perturbations , 1984 .
[2] C. Hayashi,et al. Accumulation of planetesimals in the solar nebula , 1983 .
[3] A. Cazenave,et al. Numerical experiment applicable to the latest stage of planet growth , 1982 .
[4] S. Weidenschilling,et al. Dust to planetesimals: Settling and coagulation in the solar nebula , 1980 .
[5] William K. Hartmann,et al. Planetesimals to planets: Numerical simulation of collisional evolution , 1978 .
[6] S. Weidenschilling,et al. Aerodynamics of solid bodies in the solar nebula. , 1977 .
[7] C. Hayashi,et al. Long-Term Behavior of Planetesimals and the Formation of the Planets , 1977 .
[8] Akira Fujiwara,et al. Destruction of basaltic bodies by high-velocity impact , 1977 .
[9] C. Hayashi,et al. The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula , 1976 .
[10] P. Goldreich,et al. The formation of planetesimals. , 1973 .
[11] G. Wetherill. Formation of the Terrestrial Planets , 1980 .
[12] W. Hartmann. A special class of planetary collisions - Theory and evidence , 1979 .
[13] V. Safronov,et al. Evolution of the protoplanetary cloud and formation of the earth and the planets , 1972 .