Central engine afterglow of Gamma-ray Bursts
Before 2004, nearly all GRB afterglow data could be understood in the context of the external shocks model. This situation has changed in the past two years, when it became clear that some afterglow components should be attributed to the activity of the central engine; i.e., the central engine afterglow. We review here the afterglow emission that is directly related to the GRB central engine. Such an interpretation proposed by Katz, Piran & Sari, peculiar in pre-Swift era, has become generally accepted now.
Gamma-ray bursts-radiation mechanisms nonthermal
Yi-Zhong Fan Tsvi Piran Da-Ming Wei
Purple Mountain Observatory, Chinese Academy of Science, Nanjing 210008, China National Astronomical The Racah Inst. of Physics, Hebrew University, Jerusalem 91904, Israel Purple Mountain Observatory, Chinese Academy of Science, Nanjing 210008, China National Astronomical
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
32-35
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)