Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2524l&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
LSI+61o 303 was discovered in 1977 to be a strong, variable radio source and was proposed to be the counterpart of the COS-B γ-ray source 2CG0135+01. The radio light curve exhibits outbursts whose periodicity corresponds to the optical periodicity of the orbital motion. LSI+61o 303 has been also identified as an x-ray source and an MeV γ-ray source. Long-term continuous x-ray monitoring of LSI+61o 303 by the RXTE/All-Sky-Monitor has now been carried out for a period of 5 years. These data are analyzed and the resulting time variations are summarized. The results are compared to those from radio studies and from a previous x-ray study covering a period of ten months.
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