Gamma-Rays from the Massive Binary LSI 61o+303

Details Gamma-Rays from the Massive Binary LSI 61o+303 Gamma-Rays from the Massive Binary LSI 61o+303

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2465s&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

Scientific paper

We investigate the model for gamma-ray emission from massive binary LSI 61 +303 in which a young Vela type pulsar injects relativistic e± pairs into the o radiation field of a massive Be type star. The gamma-rays are produced by e± pairs in the inverse Compton scattering (ICS) occurring in the pulsar wind zone confined by the shock formated in the collisions of the stellar and pulsar winds. We calculate these gamma-ray spectra as a function of the phase of the pulsar on its eccentric orbit around the massive star.

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