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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://ojagopokar.nm.ru/308.html ep 8rda3 драйвер скачать, http://adumerituq.nm.ru/135.html знакомства с геями, http://ojagopokar.nm.ru/275.html драйвер intel 865g windows 7,

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