Chandrasekhar, S. (1970) The evolution of the Jacobi ellipsoid by gravitational radiation Astrophysical Journal, 161 . pp. 571-578. ISSN 0004-637X
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Official URL: http://adsabs.harvard.edu/abs/1970ApJ...161..571C
Related URL: http://dx.doi.org/10.1086/150561
Abstract
The quasi-static evolution of the Jacobi ellipsoid by gravitational radiation is determined by integrating the equation that gives the rate of dissipation of the angular momentum with the constraint that the ellipsoid remains Jacobian at all times. It is found that the evolution is in the direction of increasing angular velocity toward a non-radiating state at the point of bifurcation with the Maclaurin sequence.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to American Astronomical Society. |
| ID Code: | 70806 |
| Deposited On: | 22 Nov 2011 04:37 |
| Last Modified: | 18 May 2016 16:44 |
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