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Aspects of the Collapse of Compact Objects

Published online by Cambridge University Press:  25 April 2016

R. A. Gingold
Affiliation:
Department of Mathematics, Monash University
J. J. Monaghan
Affiliation:
Department of Mathematics, Monash University

Extract

Misner Thorne and Wheeler (1973), (page 629) suggested that a freshly formed White Dwarf star of several solar masses would, if slowly — rotating, collapse to form a neutron star pancake which would become unstable and eventually produce several, possibly colliding, neutron stars.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1980

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References

Misner, C. W., Thome, K. S., and Wheeler, J. A., Gravitation, San Francisco, Freeman, W. H., p 629 (1973).Google Scholar
Canuto, V., Ann. Rev. Astron. Astrophys. 13, 335 (1975).Google Scholar
Gingold, R. A., and Monaghan, J. J., Mon. Not. R. Astron. Soc., 184, 481 (1978).Google Scholar
Tohline, J. E., Astrophys. J., 235, 866 (1980).Google Scholar