GRB 030329 光学后glow 偏振演化
天体物理学
2009-11-10 v1
摘要
我们报告了对 GRB 030329 后glow 的 31 项偏振观测，具有高信噪比和高采样频率。数据表明，该后glow 的磁场具有较小的相干长度，且主要为随机的，可能由湍流产生。
引用
@article{arxiv.astro-ph/0312089,
title = {The polarization evolution of the optical afterglow of GRB 030329},
author = {J. Greiner and S. Klose and K. Reinsch and H. M. Schmid and R. Sari and D. H. Hartmann and C. Kouveliotou and A. Rau and E. Palazzi and C. Straubmeier and B. Stecklum and S. Zharikov and G. Tovmassian and O. Barnbantner and C. Ries and E. Jehin and A. Henden and A. A. Kaas and T. Grav and J. Hjorth and H. Pedersen and R. A. M. J. Wijers and A. Kaufer and H. -S. Park and G. Williams and O. Reimer},
journal= {arXiv preprint arXiv:astro-ph/0312089},
year = {2009}
}
备注
2003 GRB Conference, Santa Fe, Oct. 2003, 1 ps-figure