The Synchrotron-self-Compton Radiation Accompanying Shallow Decaying X-Ray Afterglow： the Case of GR

• 作 者: Da-Ming Wei Yi-Zhong Fan
• 机 构: PurpleMountainObservatory,NationalAstronomicalObservatories,JointCenterforParticleNuclearPhysicsandC
• 出 处: 中国天文和天体物理学报：英文版
• 发表日期: 2007年4期
• 关键词: γ射线 喷射 爆发 辐射机制 热量 gamma-rays： bursts - ISM： jets and outflows - radiation mechan
• 基金项目: Supported by the National Natural Science Foundation of China.Acknowledgements This work is supported by the National Natural Science Foundation of China （Grants 10225314, 10233010, 10621303 and 10673

High energy emission (> tens MeV) of Gamma-Ray Bursts (GRBs) provides an important clue on the physical processes occurring in GRBs that may be correlated with the GRB early afterglow. A shallow decline phase has been well identified in about half of S