Neutron star formation in theoretical supernovae. Low mass stars and white dwarfs
Description:
The presupernova evolution of stars that form semi-degenerate or strongly degenerate O + Ne + Mg cores is discussed. For the 10 to 13 Msub solar stars, behavior of off-center neon flashes is crucial. The 8 to 10 m/sub solar stars do not ignite neon and eventually collapse due to electron captures. Properties of supernova explosions and neutron stars expected from these low mass progenitors are compared with the Crab nebula. The conditions for which neutron stars form from accretion-induced coll…
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Date:
January 1, 1986
Creator:
Nomoto, K.
Item Type:
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Partner:
UNT Libraries Government Documents Department