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Numerical Simulations of Fission

Published online by Cambridge University Press:  14 August 2015

R. H. Durisen ,
S. Yang  and
R. Grabhorn
R. H. Durisen
Affiliation:
Department of Astronomy, Swain Hall West 319, Indiana UniuersityBloomington, IN 47405, U.S.A.
S. Yang
Affiliation:
Department of Astronomy, Swain Hall West 319, Indiana UniuersityBloomington, IN 47405, U.S.A.
R. Grabhorn
Affiliation:
Department of Astronomy, Swain Hall West 319, Indiana UniuersityBloomington, IN 47405, U.S.A.

Abstract

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Recent hydrodynamic simulations indicate that gravitational torques due to spirals arms suppress binary fission in rapidly rotating polytropic fluids.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 133 - 135
Copyright
Copyright © Kluwer 1989

References

Durisen, R.H., and Gingold, R.A. (1986) “Numerical Simulations of Fission”, in Hartmann, W.K. et al. (eds.), Origin of the Moon. Lunar & Planetary Inst., Houston, pp. 487–498.Google Scholar
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