Fragmentation of a nonisothermal protostellar cloud
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference12 articles.
1. Evolution of rotating interstellar clouds. I. Numerical techniques;Black;Astrophys. J.,1975
2. The effects of rotation during star formation;Bodenheimer,1981
3. Protostellar formation in rotating interstellar clouds. I. Numerical methods and tests;Boss;Astrophys. J.,1980
4. A heuristic criterion for instability to fragmentation in rotating, interstellar clouds;Boss;Astrophy. J.,1982
5. Hydrodynamical models of presolar nebula formation;Boss;Icarus,1982
Cited by 5 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. Theory of Collapse and Protostar Formation;Interstellar Processes;1987
2. Protostellar formation in rotating interstellar clouds. V - Nonisothermal collapse and fragmentation;The Astrophysical Journal Supplement Series;1986-11
3. The Young Sun, The Early Earth and the Photochemistry of Oxygen, Ozone and Formaldehyde in the Early Atmosphere;Chemical Events in the Atmosphere and their Impact on the Environment - Proceedings of A Study Week at the Pontifical Academy of Sciences;1986
4. Three-dimensional calculations of the formation of the presolar nebula from a slowly rotating cloud;Icarus;1985-01
5. Angular momentum transfer by gravitational torques and the evolution of binary protostars;Monthly Notices of the Royal Astronomical Society;1984-08-01
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