Rapid X-ray and optical flares from Scorpius X-1

作者: L. D. Petro , H. V. Bradt , R. L. Kelley , K. Horne , R. Gomer

DOI: 10.1086/183682

关键词: AstrophysicsBinary starX-ray astronomyPlasmaFlareLight emissionX-rayTime structurePhysicsTime lagAstronomySpace and Planetary ScienceAstronomy 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.

参考文章(0)