Modeling the multi-wavelength spectrum of the gamma-ray source LSI+61**0303

Details Modeling the multi-wavelength spectrum of the gamma-ray source LSI+61**0303 Modeling the multi-wavelength spectrum of the gamma-ray source LSI+61**0303

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2532l&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

Considerable interest has centered around LSI+61o 303 since 1977 when it was discovered to be variable radio source and proposed to be the counterpart of a COS-B γ-ray source. 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. The various observations in different wavebands from radio wavelengths through to γ-rays are summarized here. A new emission model is constructed which is strongly constrained by the multi-waveband data.

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