Three-dimensional calculations of the formation of the presolar nebula from a slowly rotating cloud-Reference-Cited by-同舟云学术

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Three-dimensional calculations of the formation of the presolar nebula from a slowly rotating cloud

Published:1985-01 Issue:1 Volume:61 Page:3-9
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Boss Alan Paul

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference16 articles.

1. The effects of rotation during star formation;Bodenheimer,1981

2. Fragmentation of a nonisothermal protostellar cloud;Boss;Icarus,1983

3. Protostellar formation in rotating interstellar clouds. IV. Nonisothermal collapse;Boss;Astrophys. J.,1984

4. Angular momentum transfer by gravitational torques and the evolution of binary protostars;Boss;Mon. Not. R. Astron. Soc.,1984

5. Nucleation and condensation in the primitive solar nebula;Cameron;Icarus,1982

Cited by 17 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. Cooling and quasi-static contraction of the primitive solar nebula after gas accretion;The Astrophysical Journal;1990-07

2. The formation phase of the solar nebula;The Astrophysical Journal;1990-06

3. Equilibrium models of self-gravitating inviscid disks resulting from the collapse of rotating clouds;The Astrophysical Journal;1990-03

4. The Earth as a planet;Quo Vadimus: Geophysics for the Next Generation;1990

5. Fragmentation of Isothermal and Nonisothermal Protostellar Clouds;Astrophysics and Space Science Library;1990

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