Abstract
In the paper we present results of numerical simulations of magnetorotational model of explosion of magnetized cloud. For the simulation we used a specially developed 2D implicit numerical scheme on Lagrangian triangular grid with grid reconstruction. Our results show that due to the amplification of toroidal magnetic field component and transfer of angular momentum, a compression wave in the envelope of the cloud appears and moves through rapidly decreasing density background. This wave turns into a shock wave and pushes out part of the envelope of the star. Quantitative estimates of mass and energy carried away are given.
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Ardeljan N.V., Bisnovatyi-Kogan G.S., Kosmachevskii K.V., Moiseenko S.G., 1996a, A&AS, 115, 573
Ardeljan N.V., Bisnovatyi-Kogan G.S., Moiseenko S.G., 1996b, Ap&SS, 115, 573
Ardeljan N.V., Bisnovatyi-Kogan G.S., Popov Ju.P., Chernigovskii S.V., 1987, AZh, 64, 761
Bisnovatyi-Kogan G.S., 1970, AZh, 14, 652
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© 1998 Springer-Verlag
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Ardeljan, N.V., Bisnovatyi-Kogan, G.S., Moiseenko, S.G. (1998). Magnetorotational mechanism: 2D simulation. In: Breitschwerdt, D., Freyberg, M., Trümper, J. (eds) The Local Bubble and Beyond Lyman-Spitzer-Colloquium. Lecture Notes in Physics, vol 506. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0104710
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DOI: https://doi.org/10.1007/BFb0104710
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