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Conference Paper

Gamma-rays from PSR B1259 -63

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Kirk,  John
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Citation

Kirk, J., Ball, L., & Johnston, S. (n.d.). Gamma-rays from PSR B1259 -63. In Proceedings of the 29th International Cosmic Ray Conference.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-885B-0
Abstract
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.