Rapidly rotating neutron stars
Journal Article
·
· Phys. Rev. Lett., v. 30, no. 21, pp. 1082-1084
Models of differentially rotating neutron stars have been calculated. An upper limit to the rotational enhancement of the maximum gravitational masks is found to be about 50% when the Ostriker-Tassoul instability criterion is used. (auth)
- Research Organization:
- Lawrence Livermore Laboratory, University of California, Livermore, California, 94550
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-29-001136
- OSTI ID:
- 4417127
- Journal Information:
- Phys. Rev. Lett., v. 30, no. 21, pp. 1082-1084, Journal Name: Phys. Rev. Lett., v. 30, no. 21, pp. 1082-1084; ISSN PRLTA
- Country of Publication:
- United States
- Language:
- English
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