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Stability of an Idealised Equilibrium Model of Prominences in Rapidly-Rotating Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
We study the stability of an idealised model of stellar prominences. We find that surface fields of a few hundred gauss are required to hold them in a stable equilibrium.
- Type
- Stellar Filaments
- Information
- International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 239 - 242
- Copyright
- Copyright © Astronomical Society of the Pacific 1998