ちゅうせいしせい
中性子星
1. neutron starAstronomy
2. Neutron starA neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event. Such stars are composed almost entirely of neutrons, which are subatomic particles without electrical charge and with slightly larger mass than protons. Neutron stars are very hot and are supported against further collapse by quantum degeneracy pressure due to the Pauli exclusion principle.
Read “Neutron star” on English Wikipedia
Read “中性子星” on Japanese Wikipedia
Read “Neutron star” on DBpedia
Read “Neutron star” on English Wikipedia
Read “中性子星” on Japanese Wikipedia
Read “Neutron star” on DBpedia
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