作者: L. D. Petro , H. V. Bradt , R. L. Kelley , K. Horne , R. Gomer
DOI: 10.1086/183682
关键词: Astrophysics 、 Binary star 、 X-ray astronomy 、 Plasma 、 Flare 、 Light emission 、 X-ray 、 Time structure 、 Physics 、 Time lag 、 Astronomy 、 Space and Planetary Science 、 Astronomy and Astrophysics
摘要: A 1 second time structure in X-ray flares from Sco X-1 and simultaneous optical with structures no faster than 20 s are reported. The shortest reported scale the emission is decreased by a factor of 10, while remaining consistent parameters standard plasma model X-1. Different mechanisms for production suggested, reprocessing on surface binary companion ruled out X-ray/optical flare delay.