SS 433: 射电/X射线反相关与快速时变性质
天体物理学
2007-05-23 v1
摘要
我们简要回顾银河微类星体SS 433/W50，并提出新的RXTE光谱与时序研究。我们显示在射电闪光期间X射线强度会下降，这种行为在其他微类星体中也可见。我们还发现短时间尺度的时变性质，揭示了来自双星系统内部的辐射区。
引用
@article{arxiv.astro-ph/0210396,
title = {SS 433: Radio/X-ray anti-correlation and fast-time variability},
author = {Samar Safi-Harb and Taro Kotani},
journal= {arXiv preprint arXiv:astro-ph/0210396},
year = {2007}
}
备注
4 pages, 3 figures, mq.sty included. A higher resolution version can be found at http://aurora.physics.umanitoba.ca/~samar/4MQ/ss433/. Proceedings of the 4th Microquasar Workshop, eds. Ph. Durouchoux, Y. Fuchs and J. Rodriguez, published by the Center for Space Physics: Kolkata (in press)