SUPERORBITAL MODULATION OF X-RAY EMISSION FROM GAMMA-RAY BINARY LSI +61 303

摘要

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 a long, multi-year timescale. Using the data from the monitoring of the system by RXTE we show that the orbital phase of X-ray flares from the source varies from φX～0.35 to φX～0.75 on the uperorbital 4.6 yr timescale. Simultaneous radio observations show that periodic radio flares always lag the X-ray flare by ΔφX-R～0.2. We propose that the constant phase lag corresponds to the time of light of the high-energy particle-filled plasma blobs from inside the binary to the radio emission region at the distance of ～10 times the binary eparation distance. We put forward a hypothesis that the X-ray bursts correspond to the moments of formation of plasma blobs inside the binary system.