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(If the mass of the core exceeds the Chandrasekhar limit, electron degeneracy pressure will be unable to support its weight against the force of gravity, and the core will undergo sudden, catastrophic) |
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| − | + | If the mass of the core exceeds the Chandrasekhar limit, electron degeneracy pressure will be unable to support its weight against the force of gravity, and the core will undergo sudden, catastrophic collapse to form a neutron star or (in the case of cores that exceed the Tolman-Oppenheimer-Volkoff limit), a black hole., http://ufuvalov.nm.ru/341.html 17 ÑÑезд вкп б ÑеÑеÑаÑ, http://ufuvalov.nm.ru/411.html call centr referat, http://ufuvalov.nm.ru/196.html 12 apostolov referat, | |