Superorbital modulation of X-ray emission from gamma-ray binary LSI +61 303
arXiv:1203.1944 · doi:10.1088/2041-8205/747/2/L29
Abstract
We report the discovery of a systematic constant time lag between the X-ray and radio flares of the gamma-ray binary LSI +61 303, persistent over long, multi-year, time scale. Using the data of monitoring of the system by RXTE we show that the orbital phase of X-ray flares from the source varies from to on the superorbital 4.6 yr time scale. Simultaneous radio observations show that periodic radio flares always lag the X-ray flare by . We propose that the constant phase lag corresponds to the time of flight of the high-energy particle filled plasma blobs from inside the binary to the radio emission region at the distance ~10 times the binary separation distance. We put forward a hypothesis that the X-ray bursts correspond to the moments of formation of plasma blobs inside the binary system.
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Cited by in corpus (25)
- Gamma-ray binaries and related systems
- Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions
- Multi-wavelength Observations of the Binary System PSR B1259-63/LS~2883 around the 2014 Periastron Passage
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- Owens Valley Radio Observatory monitoring of LS I +61°303 completes three cycles of the super-orbital modulation
- Achromatic rapid flares in hard X-rays in the -ray binary LS I +61-303
- Spectral lags of flaring events in 303 from RXTE Observations