Pulsar models of the VHE γ-rays from LS 5039 and LS I+61 303

Details Pulsar models of the VHE γ-rays from LS 5039 and LS I+61 303 Pulsar models of the VHE γ-rays from LS 5039 and LS I+61 303

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..253s&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

Pulsars, Gamma-Ray, Binary And Multiple Stars

Scientific paper

We present some results of a pulsar model (including a detailed account
of the system geometry, the angular dependence of processes such as
Klein-Nishina inverse Compton and γγ absorption, and a Monte
Carlo simulation of cascading) of the high energy phenomenology of LS
5039 and LS I+61 303 and compare with recent observations.

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