Swift GRB的无色差性中断：是否有证据？
天体物理学
2010-11-11 v1
摘要
尽管Swift时代提供了γ射线暴（GRB）后glow的多波段高质量数据，但与预期相反，我们尚未完全确认标准后glow模型的最基本特征：衰减光变曲线中存在无色差性中断。我们简要回顾了迄今为止识别出的最有趣的案例。
引用
@article{arxiv.astro-ph/0612643,
title = {Achromatic Breaks for Swift GRBs: Any Evidence?},
author = {S. Covino and D. Malesani and G. Tagliaferri and S. D. Vergani and G. Chincarini and D. A. Kann and A. Moretti and L. Stella},
journal= {arXiv preprint arXiv:astro-ph/0612643},
year = {2010}
}
备注
Proceedings of the international conference Swift and GRBs: Unveiling the Relativistic Universe - Venice, 5-9 June 2006 - To appear in "Il Nuovo Cimento"