Hostname: page-component-745bb68f8f-hvd4g Total loading time: 0 Render date: 2025-01-13T06:05:43.975Z Has data issue: false hasContentIssue false
  • English
  • Français

Probing pulsar winds using inverse Compton scattering

Published online by Cambridge University Press:  12 April 2016

Lewis Ball  and
J. G. Kirk
Lewis Ball
Affiliation:
Research Centre for Theoretical Astrophysics, University of Sydney, N.S.W. 2006, Australia
J. G. Kirk
Affiliation:
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, D-69029, Heidelberg, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Part 7. The Surrounding of Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 527 - 528
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Ball, L., Kirk, J.G., 1999, Astroparticle Physics, in pressGoogle Scholar
Chernyakova, M.A., Illarionov, A.F., 1999, MNRAS, 304, 359 Google Scholar
Coe, M. J., et al., 1997, ApJS, 126, 237 Google Scholar
Dachs, J., Poetzel, R., Kaiser, D., 1989, A&AS, 78, 487 Google Scholar
Johnston, S., et al., 1996, MNRAS, 279, 1026 Google Scholar
Kirk, J.G., Ball, L., Skjæraasen, O., 1999a, Astroparticle Phys., 10, 31 Google Scholar
Kirk, J.G., Ball, L., Skjaeraasen, O., 1999b, these proceedingsGoogle Scholar
Kurucz, R.L., 1979, ApJS, 40, 1 Google Scholar