使用Chandra监控SNR 1987A的演化
天体物理学
2007-05-23 v1
摘要
我们报告了使用Chandra X射线望远镜监控SNR 1987A计划的结果。最新的Chandra数据具有高分辨率图像和光谱，表明冲击波已到达SNR西侧和东侧的致密内环。观察到的软X射线通量比三年前的通量增长得更快，最新的通量是三年前通量的四倍。
引用
@article{arxiv.astro-ph/0310374,
title = {Monitoring The Evolution of SNR 1987A with Chandra},
author = {Sangwook Park and David N. Burrows and Gordon P. Garmire and Svetozar A. Zhekov and Dick McCray},
journal= {arXiv preprint arXiv:astro-ph/0310374},
year = {2007}
}
备注
4 pages including 4 figures. To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler