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Magnetorotational Mechanism: 2D Simulation
Published online by Cambridge University Press: 12 April 2016
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.
- Type
- Part III Observations and Modeling of the Local Bubble and the SXRB
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 145 - 148
- Copyright
- Copyright © Springer-Verlag 1998