X-Ray, Gamma-Ray and Radio Observations of LSI+61 303 and the Nature of the Electron Population and of the Emission Mechanisms

Details X-Ray, Gamma-Ray and Radio Observations of LSI+61 303 and the Nature of the Electron Population and of the Emission Mechanisms X-Ray, Gamma-Ray and Radio Observations of LSI+61 303 and the Nature of the Electron Population and of the Emission Mechanisms

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2461l&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

LSI+61 303 is an unusual binary system which was discovered by its periodic 26-day radio outbursts, then subsequently identified with a COS-B gammaray source. Extensive radio and x-ray observations have been carried out since, the latter including ROSAT, ASCA, and RXTE satellite observation campaigns. It has also been identified as a CGRO/EGRET gamma-ray source. The evidence is that the radio emission is synchrotron and the x-ray through gamma-ray emission is inverse-Compton. Here the various observations are collected and used to determine the properties of the relativistic electron population.

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