Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-10-08
Astron. Rep., 2001, 45, 899-907
Astronomy and Astrophysics
Astrophysics
latex, 4 pages, 5 figures, Talk given at 5th Int. Tsessevich Conf. "Variable Stars", Odessa, Ukraine, August 2001
Scientific paper
10.1134/1.1416279
The observed mass distribution for the compact remnants of massive stars (neutron stars and black holes) and its relationship to possible mechanisms for the ejection of the envelopes of type II and Ib/c supernovae is analyzed. The conclusion is drawn that this distribution can be obtained only by a magneto-rotational mechanism for the supernovae with sufficiently long time of the field amplification, and a soft equation of state for neutron stars with limiting masses \sim1.5-1.6M_\odot. Some consequences of this hypothesis are discussed.
Postnov Konstantin A.
Prokhorov Mikhail E.
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