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Probing pulsar winds using inverse Compton scattering

  • Lewis Ball (a1) and J. G. Kirk (a2)

Abstract

We investigate the modifications to the calculations of inverse Compton scattering by the wind of pulsar B1259–63 due to the inclusion of a realistic spectrum for the target photons from the pulsar’s Be-star companion.

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Copyright

References

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Ball, L., Kirk, J.G., 1999, Astroparticle Physics, in press
Chernyakova, M.A., Illarionov, A.F., 1999, MNRAS, 304, 359
Coe, M. J., et al., 1997, ApJS, 126, 237
Dachs, J., Poetzel, R., Kaiser, D., 1989, A&AS, 78, 487
Johnston, S., et al., 1996, MNRAS, 279, 1026
Kirk, J.G., Ball, L., Skjæraasen, O., 1999a, Astroparticle Phys., 10, 31
Kirk, J.G., Ball, L., Skjaeraasen, O., 1999b, these proceedings
Kurucz, R.L., 1979, ApJS, 40, 1
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0252-9211
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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