X-rays from magnetically channeled winds of OB stars

Details X-rays from magnetically channeled winds of OB stars X-rays from magnetically channeled winds of OB stars

2008-01-30

arxiv.org/abs/0801.4780v1

Astronomy and Astrophysics

Astrophysics

2 pages; 1 figure (color, but looks fine in b/w). To appear as part of an article on the specialist session on magnetic massiv

Scientific paper

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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