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Diffusion, Winds and X-Rays from Magnetic Stars

Published online by Cambridge University Press:  14 August 2015

J. Babel
J. Babel*
Affiliation:
Switzerland, (babeljr@bluewin.ch)†

Abstract

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We propose a self-consistent approach of the CP star phenomenon and try to solve simultaneously the problems of abundance spots, wind and X-ray emission from these stars. We also discuss the periodic X-ray emission from the 07V star θ1 Orionis C and its link with Bp stars.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 674 - 675
Copyright
Copyright © Kluwer 1998

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