Daily radio variability of X-ray binaries with relativistic jets

Details Daily radio variability of X-ray binaries with relativistic jets Daily radio variability of X-ray binaries with relativistic jets

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459..445t&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Physics

1

X-Ray Binaries, Jets, Radio Emission

Scientific paper

We discussed several long daily monitoring programs with the RATAN-600 radio telescope of the sources: SS433, Cyg X-3, LSI +61°303, GRS 1915+10 at 1-22 GHz. We confirmed the correlation flaring radio emission of Cyg X-3 with hard and the anti-correlation with soft X-ray emission during the strong flare (>3 Jy) in May 1997. Powerful flaring events of SS433 were detected at six frequencies in May 1996 and in May 1999. We first detected 6.04+/-0.06 day modulation at level 10-15% from quiet flux density of SS433, that could be related with Doppler boosting in 0.26c-moving precessing and nodding jets with discrete condensations. Two flaring events near a phase 0.6 of the 26.5-day orbital period have been detected for first time at four frequencies simultaneously for the remarkable X-binary LSI +61°303 in 1998.

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