双磁星：SGR 1627-41 与 1E 1547-5408
高能天体物理现象
2009-08-05 v1
摘要
我们报告了通过对银河系源 SGR 1627-41 和 1E 1547-5408 进行目标观测所获得的最新结果。这两个瞬变源呈现出若干相似性，支持将反常X射线脉冲星和软伽马射线重复暴解释为单一类别的强磁化中子星。
引用
@article{arxiv.0908.0414,
title = {The Twin Magnetars: SGR 1627-41 and 1E 1547-5408},
author = {S. Mereghetti and A. Tiengo and P. Esposito and G. Vianello and A. De Luca and D. Gotz and G. Weidenspointner and A. von Kienlin and G. L. Israel and L. Stella and N. Rea and R. Turolla and S. Zane},
journal= {arXiv preprint arXiv:0908.0414},
year = {2009}
}
备注
To be published in the proceedings of the conference "Neutron Stars and Gamma Ray Bursts: Recent Developments and Future Directions" - March 30 - April 4, 2009 (Cairo and Alexandria, Egypt)