Runaway planetary growth with collision rate in the solar gravitational field-Reference-Cited by-同舟云学术

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Runaway planetary growth with collision rate in the solar gravitational field

Published:1990-06 Issue:2 Volume:85 Page:499-511
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Ohtsuki Keiji,Ida Shigeru

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference19 articles.

1. Planetesimals to planets: Numerical simulation of collisional evolution;Greenberg;Icarus,1978

2. Accretion rates of protoplanets;Greenzweig,1990

3. Long-term behavior of planetesimals and the formation of the planets;Hiyashi;Publ. Astron. Soc. Japan,1977

4. Stirring and dynamical friction rates of planetesimals in the solar gravitational field;Ida,1990

5. Collisional probability of planetesimals revolving in the solar gravitational field. III;Ida;Astron. Astrophys.,1989

Cited by 30 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. EVAPORATION OF ICY PLANETESIMALS DUE TO BOW SHOCKS;The Astrophysical Journal;2013-01-30

2. Accretion of planetary embryos in the inner and outer solar system;Physica Scripta;2008-07-16

3. Production of trans-Neptunian binaries through chaos-assisted capture;Monthly Notices of the Royal Astronomical Society;2007-07-21

4. Models of the collisional damping scenario for ice-giant planets and Kuiper belt formation;Icarus;2007-07

5. On some aspects of the stirring rate of planetesimal velocities by a protoplanet;Monthly Notices of the Royal Astronomical Society;2007-06-21

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