  The high-energy gamma-ray light curve of the binary system PSR B1259 -63, is
computed using the approach that successfully predicted the spectrum at
periastron. The simultaneous INTEGRAL and H.E.S.S. spectra taken 16 days after
periastron currently permit both a model with dominant radiative losses, high
pulsar wind Lorentz factor and modest efficiency as well as one with dominant
adiabatic losses, a slower wind and higher efficiency. In this paper we shown
how the long-term light curve may help to lift this degeneracy.

Astrophysics