Sokolov2006 用致密星做GRB的中心源模型 2

主要内容:
提了一个模型, 认为伽玛暴(长暴)全部与超新星成协. 但是张角很小(只有0.x度), 幅射总能量小于10^49erg, 而不是现在估计的10^51erg.

可是喷流拐折时间就应该很早呃.

查了一下, 有这么多SGR?　1806-20. 1900+14. 0526-66. 1627-41. 1801-23

精彩摘抄:


文章信息:
astro-ph/0607644
Observational Constraints on the Angular and Spectral Distributions of Photons in Gamma-Ray Burst Sources
Authors: V. V. Sokolov (1), G. S. Bisnovatyi-Kogan (2), V. G. Kurt (3), Yu. N. Gnedin (4), Yu. V. Baryshev (5) ((1) Special Astrophysical Observatory, Russian Academy of Sciences, (2) Space Research Institute, Moscow, (3) Astro-Space Center, Lebedev Physical Institute, (4) Main Astronomical Observatory, Pulkovo, (5) Astronomical Institute, St. Petersburg State University)
Comments: 15 pages, no figures, no tables
Journal-ref: Astronomy Reports, 2006, Vol.50, No.8, pp.612-625