Formation and Radiation Acceleration of Pair Plasmoids Near Galactic Black Holes
Formation and Radiation Acceleration of Pair Plasmoids Near Galactic Black Holes
复制标题
银河系黑洞附近等离子体团对的形成和辐射加速
DOI：
10.1086/176833
复制
发表时间：
1995
期刊：
影响因子：
--
通讯作者：
Huijun Liang
中科院分区：
文献类型：
--
作者：
Huijun Liang
We study quantitatively the formation and radiation acceleration of electron-positron pair plasmoids produced by photon-photon collisions near Galactic black holes (GBHs). The terminal ejecta velocity is found to be completely determined by the total disk luminosity, proton loading factor and disk size, with no dependence on the initial velocity. We discuss potential applications to the recently discovered Galactic superluminal sources GRS1915, GROJ1655 and possibly other GBHs.
