Hostname: page-component-5c6d5d7d68-lvtdw Total loading time: 0 Render date: 2024-08-07T09:20:46.128Z Has data issue: false hasContentIssue false
  • English
  • Français

Can Stellar Atmospheres be in Quasi-Static Equilibrium in the Presence of Magnetic Fields?

Published online by Cambridge University Press:  14 August 2015

Kyoji Nariai
Kyoji Nariai*
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo Mitaka Tokyo 181, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Among the observational astronomers it is quite customary to assume potential magnetic fields in calculating the strength and the direction of the magnetic fields on the stellar surface. People use this assumption because

  1. 1. it is easy to calculate,

  2. 2. it is possible to fit the observations with the calculations to some extent using the parameters inherent to the model,

  3. 3. at a first glance, there is no difficulty in assuming both potential magnetic fields and static stellar atmosphere because they do not interact each other (except at the pole).

Type
Session 6: Effect of Rotation and Magnetic Field in Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 276 - 277
Copyright
Copyright © Reidel 1981