Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-18T05:24:42.009Z Has data issue: false hasContentIssue false
  • English
  • Français

Aspects of the Collapse of Compact Objects

Published online by Cambridge University Press:  25 April 2016

R. A. Gingold  and
J. J. Monaghan
R. A. Gingold
Affiliation:
Department of Mathematics, Monash University
J. J. Monaghan
Affiliation:
Department of Mathematics, Monash University
Get access Rights & Permissions [Opens in a new window]

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
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 49 - 50
Copyright
Copyright © Astronomical Society of Australia 1980

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

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