Gamma-ray emission from pulsar/massive-star binaries
arXiv:0908.3616 · doi:10.1017/S1743921310008501
Abstract
I present a review of the main phenomenological properties at high energies related to massive gamma-ray binaries and I discuss some aspects of pulsar models for these objects.
Invited review to the IAU GA JD03, August 2009, to be published in Highlights of Astronomy, T. M. Belloni et al. (eds.), 5 pages