Ryde2006 伽玛暴的光球层 3

主要内容:
考虑了光球层的重要性, 提出E_p应该是光球层热温度的peak经过Lorentz boosting之后的. 并推导了Amati关系以及hardness-intensity correlation (HIC).

精彩摘抄:
GRB960530的谱, 热幅射+密率. E_p=100keV, 是热成份部分的.

文章信息:
astro-ph/0608363
Gamma-Ray Burst Spectral Correlations: Photospheric and Injection Effects Authors: Felix Ryde, Claes-Ingvar Bjornsson, Yuki Kaneko, Peter Meszaros, Robert Preece, Milan Battelino
Comments: ApJ accepted, acknowledgement added