作者: P. Bodenheimer , R. E. Taam
DOI: 10.1086/162049
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摘要: The evolution of a double-core configuration consisting 16 M/sub sun/ supergiant and an immersed 1 neutron star is investigated with two-dimensional numerical hydrodynamic calculation. When the orbiting deep within envelope, frictional effects deposit energy rapidly enough to drive expansion that preferentially directed in equatorial plane. A calculation which follows expanding material surface shows about accelerated escape velocity suggests ejection entire envelope could occur. calculations are compared previous one-dimensional evolution.