OB 星磁约束星风产生的 X 射线
天体物理学
2008-02-01 v1
摘要
具有强辐射驱动星风和大尺度磁场的 OB 星，通过磁约束星风激波（MCWS）机制产生强且硬的 X 射线发射。在这篇简短的论文中，我描述了 OB 星中 MCWS 机制的四种独立 X 射线诊断方法，并将其应用于原初型年轻 O 星猎户座θ¹C（theta-1 Ori C）。
引用
@article{arxiv.0801.4780,
title = {X-rays from magnetically channeled winds of OB stars},
author = {David H. Cohen},
journal= {arXiv preprint arXiv:0801.4780},
year = {2008}
}
备注
2 pages; 1 figure (color, but looks fine in b/w). To appear as part of an article on the specialist session on magnetic massive stars held prior to IAU Symposium 250, "Massive Stars as Cosmic Engines," Kauai, HI, December 2007; eds. Bresolin, Crowther, & Puls, Cambridge University Press, 2008