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Diffusion, Winds and X-Rays from Magnetic Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
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
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- Copyright
- Copyright © Kluwer 1998