Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-26T05:17:15.008Z Has data issue: false hasContentIssue false
  • English
  • Français

An Inverse Compton Scattering Model for the Spectra of X-ray Pulsars

Published online by Cambridge University Press:  04 August 2017

G.J. Qiao ,
X.J. Wu ,
H. Chen  and
X.Y. Xia
G.J. Qiao
Affiliation:
Geophysics Department, Peking University, Peking, China
X.J. Wu
Affiliation:
Geophysics Department, Peking University, Peking, China
H. Chen
Affiliation:
Geophysics Department, Peking University, Peking, China
X.Y. Xia
Affiliation:
Department of Physics, Tianjin Normal University, Tianjin, China

Extract

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.

Many observations have been reported in the field of X-ray pulsars, but the mechanism for X-ray emission is not well understood. The X-ray spectra can not be simply described in terms of blackbody or thermal bremsstralung. The high-energy cutoff could be due to cyclotron absorption in high (≧1012 Gauss) magnetic fields. For the lower energy it can be fitted by a power law with energy index α.

Type
II. Accretion Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 248
Copyright
Copyright © Reidel 1987 

References

Herold, H.: 1979, Phys. Rev., D19, 2868.Google Scholar
Sutherland, P.G.: 1979, Fundamentals of Cosmic Physics, 4, 95.Google Scholar