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  The high-energy light curve of PSR B1259-63

Kirk, J., Ball, L., & Johnston, S. (2005). The high-energy light curve of PSR B1259-63. In T. B. e. al. (Ed.), Astrophysical sources of high energy particles and radiation (pp. 286-289). American Institute of Physics.

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 Creators:
Kirk, John1, Author           
Ball, Lewis2, Author
Johnston, S.2, Author
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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 Abstract: 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. ©2005 American Institute of Physics

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Language(s): eng - English
 Dates: 2005-11
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 250293
DOI: 10.1063/1.2141882
 Degree: -

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Title: Astrophysical sources of high energy particles and radiation
Place of Event: Torun, Poland
Start-/End Date: 2005-06-20 - 2005-06-24

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Title: Astrophysical sources of high energy particles and radiation
Source Genre: Proceedings
 Creator(s):
al., Tomasz Bulik et., Editor
Affiliations:
-
Publ. Info: American Institute of Physics
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 286 - 289 Identifier: -

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Title: AIP Conference Proceedings
Source Genre: Series
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Pages: - Volume / Issue: 801 Sequence Number: - Start / End Page: - Identifier: -