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- W2020443341 abstract "We report on a study of GS 1826–238 using all available Rossi X-Ray Timing Explorer observations, concentrating on the behavior of the hard X-rays during type-I bursts. We find a hard X-ray shortage at 30–50 keV prompted by the shower of soft X-rays coming from type-I bursts. This shortage happens with a time delay after the peak of the soft flux of 3.6 ± 1.2 s. The behavior of hard X-rays during bursts indicates cooling and reheating of the corona, during which a large amount of energy is required. We speculate that this energy originates from the feedback of the type-I bursts to the accretion process, resulting in a rapid temporary increase of the accretion rate." @default.
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- W2020443341 date "2014-01-24" @default.
- W2020443341 modified "2023-10-05" @default.
- W2020443341 title "THE HARD X-RAY SHORTAGES PROMPTED BY THE CLOCK BURSTS IN GS 1826-238" @default.
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- W2020443341 doi "https://doi.org/10.1088/0004-637x/782/1/40" @default.
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