Jets in X-Ray Binaries
Jets in X-Ray Binaries
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DOI：
10.1007/978-94-009-3927-1_6
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发表时间：
1987
期刊：
影响因子：
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通讯作者：
H. Ögelman
中科院分区：
文献类型：
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作者：
H. Ögelman
三个银河系的X射线双星，显示喷流的证据，天蝎座X-1，天鹅座X-3，和SS 433的检查。SS 433是唯一一个在从射电到伽马射线的所有波长上都显示出丰富喷流特征的源; Sco X-1和Cyg X-3的喷流只在射电区域很明显。三个系统的观测功能，作为X射线双星，总结和比较。一个可能的共同模型的中央引擎，涉及一个快速旋转的中子星星与弱表面场（Bs <$109高斯），概述。
The three galactic X-ray binaries that show evidence for jets, Sco X-1, Cyg X-3, and SS433 are examined. SS433 is the only source that shows rich jet features in all wavelengths from radio to gamma rays; the jets of Sco X-1 and Cyg X-3 are only evident in the radio region. Observational features for the three systems, as X-ray binaries, are summarised and compared. A possible common model for the central engine, involving a fast spinning neutron star with weak surface field (Bs≲109gauss), is outlined.