Convective instability in the prompt explosion model of Type-II supernovae

Details Convective instability in the prompt explosion model of Type-II supernovae Convective instability in the prompt explosion model of Type-II supernovae

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22..161z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 2, p. 161-165.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We examined convective instability in the prompt-explosion model of SN II during the iron core collapse, rebound and shock propagation stages. We found the appearance of finger-type convection in the inner region of the core, of Schwarzschild convection in the outer region, and of Ledoux convection in the transition region between the sound-velocity point and the neutron-trapping sphere. The interval 0.74-0,91 Msolar proves to be an active region of convective instability.

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