Turbulence, Magnetic Field and Diffusive Synchrotron Radiation
In this paper, we study the perturbative treatment of Diffusive Synchrotron Radiation. The random and small-scale magnetic field may be generated by the turbulence. We find that the multi-band spectrum of the knot in Cen A produced by DSR is well constrained by the feature of stochastic magnetic field.
radiation mechanisms nonthermal--galaxies jet--galaxies active--galaxies individual (Cen A)-turbulence
Jirong Mao Jiancheng Wang
Yunnan Observatory, National Astronomical Observatories, Chinese Academic of Sciences, P. O. Box 110, Kunming, Yunnan Province, 650011, China
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
414-416
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)