The oscillations and the stability of rotating masses with magnetic fields. III.
Journal Article
·
· Astrophys. J., v. 181, no. 2, pp. 519-521
OSTI ID:4418996
It is shown that when a magnetic field is present along the axis of rotation, the point of bifurcation, where the Jacobi ellipsoids branch off from the Maclaurin spheroids, occurs at a value of eccentricity which is higher than the value (e=0.81267) that obtains in the absence of a magnetic field. This is in contrast to the effect of a toroidal magnetic field which, as has been shown earlier, leaves the point of bifurcation unaffected. (auth)
- Research Organization:
- Department of Mathematics, Panjab University, Chandigarh, India
- NSA Number:
- NSA-29-001148
- OSTI ID:
- 4418996
- Journal Information:
- Astrophys. J., v. 181, no. 2, pp. 519-521, Journal Name: Astrophys. J., v. 181, no. 2, pp. 519-521; ISSN ASJOA
- Country of Publication:
- United States
- Language:
- English
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