Magnetorotational Supernova Explosion - 2D Numerical Simulation

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dc.creatorArdeljan, N. V.
dc.creatorBisnovatyi-Kogan, G. S.
dc.creatorMoiseenko, S. G.
dc.date1997-07-22
dc.date.accessioned2026-07-07T02:23:52Z
dc.date.available2026-07-07T02:23:52Z
dc.descriptionResults of 2D numerical simulation of magnetorotational mechanism of supernova explosion are presented. It is shown that due to the differential rotation of the star toroidal component of magnetic field appears and grows with time. Angular momentum transfers outwards by the toroidal magnetic field. With the evolution of the process part of the envelope of the star is throwing away. The amount of thrown away mass and energy are estimated. The results of the simulation are qualitatively correspond to supernova explosion picture.
dc.description6 pages, 8 figures, paspconf.sty, epsf.sty, LaTeX
dc.identifierhttps://arxiv.org/abs/astro-ph/9707245
dc.identifierhttp://arxiv.org/abs/astro-ph/9707245
dc.identifierProc. of the Int. Workshop "SN1987A: Ten Years After", La Serena, Chile, February, 1997
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11416
dc.subjectAstrophysics
dc.titleMagnetorotational Supernova Explosion - 2D Numerical Simulation
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