作者: Mark Strickman
DOI: 10.1063/1.1303207
关键词: Duty cycle 、 Astronomy 、 Physics 、 Extrapolation 、 X-ray binary 、 Emission spectrum 、 Astrophysics 、 X-ray 、 Accretion (meteorology) 、 X-ray astronomy 、 Thermal radiation
摘要: CGRO/OSSE observations of the bright LMXB Sco X-1 have resulted in discovery transient episodes hard X-ray emission extending to energies above 200 keV. During these periods, spectrum 80 keV deviates significantly from extrapolation soft thermal observed at lower energies. The intervals last ∼4-days with a duty cycle ∼30%. Using RXTE/ASM data same establish state on color-color diagram “Z” is progress, but preliminary results indicate that occur over limited range mass accretion rates.