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(Owning to without unified and authoritative hospital standardization data dictionaries, as well as different HIS developed by different companies with different codes and standards, two bad results co) |
(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://owupysyj.land.ru/376.html кÑпиÑÑ ÑÑÑÐ±Ð¾Ð»ÐºÑ pokerstars, http://owupysyj.land.ru/117.html kupit futbolku kreativnyi dizain, http://owupysyj.land.ru/274.html кÑпиÑÑ ÑÑÑÐ±Ð¾Ð»ÐºÑ Ñ Ð²Ð¸ÐºÐ¸Ð½Ð³Ð¾Ð¼, | |
Revision as of 01:48, 19 January 2011
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://owupysyj.land.ru/376.html кÑпиÑÑ ÑÑÑÐ±Ð¾Ð»ÐºÑ pokerstars, http://owupysyj.land.ru/117.html kupit futbolku kreativnyi dizain, http://owupysyj.land.ru/274.html кÑпиÑÑ ÑÑÑÐ±Ð¾Ð»ÐºÑ Ñ Ð²Ð¸ÐºÐ¸Ð½Ð³Ð¾Ð¼,
