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arXiv · 0801.4780

X-rays from magnetically channeled winds of OB stars

David H. Cohen
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Abstract

OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong and hard X-ray emission via the Magnetically Channeled Wind Shock (MCWS) mechanism. In this brief paper, I describe four separate X-ray diagnostics of the MCWS mechanism in OB stars, with applications to the prototype young O star, theta-1 Ori C.

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David H. Cohen. 2008-01-30. X-rays from magnetically channeled winds of OB stars. https://arxiv.org/abs/0801.4780

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