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- W2000847423 abstract "We present the results of a study with the emph{Swift} Burst Alert Telescope in the 14 -- 195 keV range of the long-term variability of 5 low mass X-ray binaries with reported or suspected super-orbital periods -- 4U 1636-536, 4U 1820-303, 4U 1916-053, Cyg X-2 and Sco X-1. No significant persistent periodic modulation was detected around the previously reported periods in the 4U 1916-053, Cyg X-2 or Sco X-1 light curves. The $sim$170 d period of 4U 1820-303 was detected up to 24 keV, consistent with variable accretion due to the previously proposed triple system model. The $sim$46 d period in 4U 1636-536 was detected up to 100 keV, with the modulation in the low and high energy bands found to be phase shifted by $sim180^circ$ with respect to each other. This phase shift, when taken together with the near-coincident onset of the $sim$46 d modulation and the low/hard X-ray state, leads us to speculate that the modulation could herald transient jet formation." @default.
- W2000847423 created "2016-06-24" @default.
- W2000847423 creator A5001708263 @default.
- W2000847423 creator A5007049450 @default.
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- W2000847423 date "2009-02-11" @default.
- W2000847423 modified "2023-10-07" @default.
- W2000847423 title "Superorbital variability in hard X-rays" @default.
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- W2000847423 doi "https://doi.org/10.1111/j.1365-2966.2008.14167.x" @default.
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