Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-05T10:03:36.981Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray and Gamma-ray Radiation from the Switched-off Radiopulsars

Published online by Cambridge University Press:  04 August 2017

A. I. Tsygan
A. I. Tsygan*
Affiliation:
A.F. Ioffe Institute of Physics and Technology, Leningrad, USSR

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.

It is shown that pulsars that have ceased to generate electron-positron pairs (switched-off radiopulsars) may be the sources of X-ray and γ-ray radiation. The magnetic dipole radiation from these rotating neutron stars is transformed near the “light radius” into hard radiation by the plasma that is created due to ionization of interstellar neutral hydrogen.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 505 - 507
Copyright
Copyright © Reidel 1983 

References

Ferrari, A., Trussoni, E., 1974, Astronomy and Astrophysics, 36, 267.Google Scholar
Glen, G., Sutherland, P., 1980. Astrophys. J., 239, 671.CrossRefGoogle Scholar
Manchester, R.N., Taylor, J.H., 1977. Pulsars. (San Francisco: Freeman).Google Scholar
Ruderman, M.A., Sutherland, P.G., 1975. Astrophys. J., 196, 51.CrossRefGoogle Scholar
Smith, F.G., 1977. Pulsars. (Cambridge: Cambridge University Press).Google Scholar
Sturrock, P.A., 1971. Astrophys. J., 164, 529.CrossRefGoogle Scholar
Tsygan, A.I., 1980. Sov. Astrophys. J., 57, 73.Google Scholar
Vladimirsky, B.M., 1981. Conf. Papers of 17th Internat. Cosmic Ray Conference, Paris, Vol. 1, 38.Google Scholar