X-rays from magnetically channeled winds of OB stars
| dc.creator | Cohen, David H. | |
| dc.date | 2008-01-30 | |
| dc.date.accessioned | 2026-07-07T08:57:26Z | |
| dc.date.available | 2026-07-07T08:57:26Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/0801.4780 | |
| dc.identifier | http://arxiv.org/abs/0801.4780 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146967 | |
| dc.subject | Astrophysics | |
| dc.title | X-rays from magnetically channeled winds of OB stars | |
| dc.type | text |