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  Modelling the gamma-ray emission from PSR B1259

Kirk, J. G., Ball, L., & Johnston, S. (2005). Modelling the gamma-ray emission from PSR B1259. In B. S. Acharya, S. Gupta, & P. Jagadeesan (Eds.), Proceedings of the 29th International Cosmic Ray Conference (pp. 131-134). Navy Nagar, Colaba, Mumbai, MH-40005: Tata Institute of Fundamental Research.

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 Creators:
Kirk, J. G.1, Author           
Ball, Lewis2, Author
Johnston, S.2, Author
J. Kirk, Editor  
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Australia Telescope National Facility, CSIRO, PO Box 276, Parkes, NSW 2870, Australia Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia, ou_persistent22              

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Free keywords: gamma-ray astronomy
 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 nd 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 ef ciency as well as one with dominant adiabatic losses, a slower wind and higher ef ciency. Additional, simultaneous, X-ray and TeV data sets are needed to lift this degeneracy.

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Language(s): eng - English
 Dates: 2005-12
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 282112
 Degree: -

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Title: 29th International Cosmic Ray Conference
Place of Event: Pune, India
Start-/End Date: 2005-01-03 - 2005-08-10

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Title: Proceedings of the 29th International Cosmic Ray Conference
Source Genre: Proceedings
 Creator(s):
Acharya, B. Sripathi, Editor
Gupta, Sunil, Editor
Jagadeesan, P., Editor
Affiliations:
-
Publ. Info: Navy Nagar, Colaba, Mumbai, MH-40005 : Tata Institute of Fundamental Research
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 131 - 134 Identifier: -