围绕黑洞和中子星的吸积过程：导向性盘范式
天体物理学
2007-05-23 v1
摘要
我们综述了包括吸积盘模型的研究，讨论了离心压支撑的高密度区域接近致密天体对发射光谱的影响。我们指出，黑洞候选体的平稳与非平稳光谱特性（如低和高状态、准周期振荡、X 射线新星的静止和上升阶段等）可以被 satisfactory 解释。
引用
@article{arxiv.astro-ph/9703052,
title = {Accretion Processes Around Black Holes And Neutron Stars: Advective Disk Paradigm},
author = {Sandip K. Chakrabarti},
journal= {arXiv preprint arXiv:astro-ph/9703052},
year = {2007}
}
备注
13 Latex pages including figures. Macros included. To appear in `Perspective of High Energy Astrophysics', the proceedings of the Golden Jubilee International Colloquium of TIFR (8/96). Eds. P.C. Agarwal et al