Stability of rotating supermassive stars in presence of dark matter background
Preprint
- 24 December 1997
Abstract
Stability of supermassive stars embedded in hot dark matter is investigated on the base of the energetic method. Stability effect of dark mater is compared with rotational stabilization and preference of the last factor is advocated.Keywords
All Related Versions
- Version 1, 1997-12-24, ArXiv
- Published version: The Astrophysical Journal, 497 (2), 559.
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