AbstractStrange stars with low masses are suggested to exist in reality, the origin of which could be via accretion-induced collapse of white dwarfs. Such a strange star is likely bare, and would thus spin very fast, even to a period of <0.1ms. Strange stars with low masses may differ from those with solar masses in various astrophysical appearances. Observations to test this “low-mass” idea are proposed.
Low-mass bare strange stars
Advances in Space Research ; 37 , 10 ; 1992-1995
2005-10-17
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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