Gamma-rays from PSR B1259 -63
天体物理学
2016-08-30 v1
摘要
The high-energy gamma-ray emission discovered using the H.E.S.S. telescopes from the binary system PSR B1259 -63, is modelled using an extension of the approach that successfully predicted it. We find that the simultaneous INTEGRAL and H.E.S.S. data 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. Additional, simultaneous, X-ray and TeV data sets are needed to lift this degeneracy.
引用
@article{arxiv.astro-ph/0509899,
title = {Gamma-rays from PSR B1259 -63},
author = {J. G. Kirk and Lewis Ball and S. Johnston},
journal= {arXiv preprint arXiv:astro-ph/0509899},
year = {2016}
}
备注
4 pages, to appear in: Proceedings of the 29th International Cosmic Ray Conference, Pune (2005)