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- W2494779427 abstract "Abstract Emission mechanisms of the iron K α -lines in X-ray binaries are discussed in relation with the characteristic temperature T x of continuum radiation thereof. The 6.7 keV line is ascribed to radiative recombination followed by cascades in a corona of ∼ 100 eV formed above the accretion disk. This mechanism is attained for T x ≲ 10 keV as observed for low mass X-ray binaries. The 6.4 keV line observed for binary X-ray pulsars with T x > 10 keV is likely due to fluorescence outside the He II ionization front." @default.
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- W2494779427 date "1988-01-01" @default.
- W2494779427 modified "2023-09-27" @default.
- W2494779427 title "Iron K-Line Emission from X-Ray Binaries" @default.
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- W2494779427 doi "https://doi.org/10.1017/s0252921100107389" @default.
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