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- W2135280216 abstract "The characteristics of supermassive ‘stars’ consisting of self-gravitating degenerate neutrino (or neutralino) matter are studied with particular emphasis on fermion masses around 17 keV/c2. Such compact dark objects could be as massive as 109.5 to 1o6.5 solar masses, with radii of about one to ten light days; they might thus mimic phenomena that are expected around the supermassive black holes recently purported at the centres of some galaxies and quasi-stellar objects." @default.
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- W2135280216 date "1993-05-01" @default.
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- W2135280216 title "Supermassive neutrino stars and galactic nuclei" @default.
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- W2135280216 doi "https://doi.org/10.1016/0370-2693(93)91141-9" @default.
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