Deutsches Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany.
Science. 2014 Jan 3;343(6166):42-7. doi: 10.1126/science.1242353. Epub 2013 Nov 21.
The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of these unique astrophysical sources. GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest γ-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB. Temporal and spectral analyses of GRB 130427A challenge the widely accepted model that the nonthermal high-energy emission in the afterglow phase of GRBs is synchrotron emission radiated by electrons accelerated at an external shock.
费米伽马射线太空望远镜搭载的大面积望远镜对异常明亮的伽马射线暴 (GRB) 130427A 的观测结果对这些独特的天体物理源的性质提供了限制。GRB 130427A 的流量最大、最高能光子(95GeV)、最长γ射线持续时间(20 小时)和从 GRB 观测到的各向同性能量释放中最大的之一。GRB 130427A 的时间和光谱分析挑战了广泛接受的模型,即 GRB 余辉阶段的非热高能发射是由外部激波加速的电子辐射的同步辐射。