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Neutron-star formation in the carbon-detonation supernova. (1973)

Buchler, J.-R. ; Wheeler, J. C. ; Barkat, Z. K.

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Publication Date: 2019-06-27

Description: Neutrino losses, such as those driven by the convective Urca process, may affect the evolution of stars in the mass range from 4 to 8 solar masses so as to lead to collapse of their degenerate carbon/oxygen cores. A corresponding hydrodynamic model is computed which leads to the formation of a 1.3 to 1.4 solar mass neutron star with the expulsion of a small fraction of the mass, about 0.l solar mass at about 20,000 km/sec into the overlying hydrogen envelope. This sets the stage for the Ostriker-Gunn mechanism in which Type II supernovae and pulsars are formed.

Keywords: SPACE SCIENCES

Type: Astrophysical Journal; 184; Sept. 15

Format: text

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