Be/X射线瞬变源的 X 射线外冲
天体物理学
2007-05-23 v1
摘要
我们基于长期多波段监测和赤道盘模型，提出了一种解释Be/X射线二体行为的新方案。双星系统中质子星的周边赤道盘因潮汐和共振效应而被截断。系统的几何结构和黏性程度决定了是否存在I型X射线外冲。强烈扰动的赤道盘与中子星相互作用可产生II型X射线和光学外冲。
引用
@article{arxiv.astro-ph/0011406,
title = {The X-ray outbursts of Be/X-ray transients},
author = {Ignacio Negueruela and Atsuo T. Okazaki},
journal= {arXiv preprint arXiv:astro-ph/0011406},
year = {2007}
}
备注
Slightly enlarged version of paper appearing in Proceedings of IAU Colloq 175, eds Smith M.A. et al., ASP Conference Series 214. "The Be phenomenon in early-type stars", p. 713-718. Extended introduction and bibliography, one extra figure. LaTeX file, 3 figs (one in colour, prints fine in B&W);uses paspconf.sty