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- W2152576411 abstract "From the longest monitoring of LS I +61 303 done to date by the Rossi X-ray Timing Explorer (RXTE) we found evidence for the long-sought, years- long modulation in the X-ray emission of the source. The time evolution of the modulated fraction in the orbital lightcurves can be well fitted with a sinusoidal function having a super-orbital period of 1667 days, the same as the one reported in non-contemporaneous radio measurements. However, we have found a 281.8 pm 44.6 days shift between the super-orbital variability found at radio frequencies extrapolated to the observation time of our campaign and what we found in the super-orbital modulation of the modulated fraction of our X-ray data. We also find a super-orbital modulation in the maximum count rate of the orbital lightcurves, compatible with the former results, including the shift." @default.
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- W2152576411 date "2011-12-13" @default.
- W2152576411 modified "2023-09-25" @default.
- W2152576411 title "UNVEILING THE SUPER-ORBITAL MODULATION OF LS I +61°303 IN X-RAYS" @default.
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- W2152576411 doi "https://doi.org/10.1088/2041-8205/744/1/l13" @default.
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