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Self-Similar MHD Collimated Outflows
Published online by Cambridge University Press: 12 April 2016
Abstract
We present a class of steady axisymmetric MHD solutions, self-similar in the meridional direction, that are suitable to model collimated winds accelerated in the potential well of a spherical object.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 816 - 817
- Copyright
- Copyright © Astronomical Society of the Pacific 1997