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

X-rays from magnetically channeled winds of OB stars