Hostname: page-component-669899f699-tzmfd Total loading time: 0 Render date: 2025-04-29T12:36:46.398Z Has data issue: false hasContentIssue false
  • English
  • Français

To explain Crab pulsar emission by ICS Model

Published online by Cambridge University Press:  12 April 2016

J.L. Han ,
B. Zhang ,
G.J. Giao  and
R.X. Xu
J.L. Han
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, China
B. Zhang
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
G.J. Giao
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
R.X. Xu
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China

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.

Primary results of our recent work show that radio, infrared and optical, X-ray and γ-ray emission of Crab pulsar might be explained by Inverse Compton Scattering (ICS) mechanism.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 183 - 184
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Dermer, C., 1990, ApJ 360, 197 CrossRefGoogle Scholar
Moffett, D.A., Hankins, T.H., 1996, ApJ, in pressGoogle Scholar
Middleditch, J., Pennypacker, C., Burns, M.S., 1983, ApJ 273, 261 Google Scholar
Qiao, G.J., 1988, in: High Energy Astrophysics, Bonner, G.B. (ed), Springer-Verlag, p.88 Google Scholar
Qiao, G.J., Zhang, B., 1996, A.&A 306, L5 Google Scholar
Sturner, S.J., 1995, ApJ 446, 292 CrossRefGoogle Scholar
Urpin, V.A., Shalybkov, D.A., 1995, A&A 294, 117 Google Scholar
Zavlin, V.E., Pavlov, G.G., Shibanov, Yu.A., Ventura, J., 1995, A&A 297, 441 Google Scholar
Zhang, B., Qiao, G.J., 1995, A&A, in pressGoogle Scholar