General Relativistic Radiative Transfer
We present two formulations for general relativistic relativistic transfer for astrophysical systems. The first considers absorption and emission only, and the second includes also scattering. We use these formulations to calculate emission from relativistic accretion disks and tori around rotating black holes.
raditive tranfer scattering-relativity and gravitation-accretion and accretion disks-black holes-active galactic nuclei
Kinwah Wu Steven V. Fuerst
MSSL, University College London, Holmbury St Mary, Surrey RH5 6NT, United Kingdom KIPAC, Stanford University, Stanford, CA 94305, USA
国际会议
紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)
安徽黄山
英文
411-413
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)