Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-26T22:22:36.451Z Has data issue: false hasContentIssue false
  • English
  • Français

The Pulsar Magnetic Window

Published online by Cambridge University Press:  14 August 2015

C. S. Shukre  and
V. Radhakrishnan
C. S. Shukre
Affiliation:
Raman Research Institute, Bangalore-560 080, India
V. Radhakrishnan
Affiliation:
Raman Research Institute, Bangalore-560 080, India

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.

Triggering of the spark discharges in the Ruderman and Sutherland model by background gamma rays is shown to be effective only within a narrow range of neutron star magnetic fields centred on 2.5 × 1012 gauss. This calculated range of field strengths is in good agreement with ‘observed’ values, suggesting that (a) such triggering is operative, and (b) that neutron stars with much stronger fields do not function as pulsars.

Type
II. Radio Emission Mechanism
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 103 - 105
Copyright
Copyright © Reidel 1981 

References

Gullahorn, G. and Rankin, J.M.: 1978, Astron. J. 83, pp. 1219–1224.Google Scholar
Manchester, R.N., Goss, W.M., Newton, L.M., and Hamilton, P.A.: 1976, Proc. Astron. Soc. Australia 3, pp. 81–83.Google Scholar
Newton, L.M., Manchester, R.N., and Cooke, D.J.: 1980, CSIRO RPP. No. 2380.Google Scholar
Ruderman, M.A. and Sutherland, P.G.: 1975, Astrophys. J. 196, pp. 51–72.Google Scholar
Shukre, C.S. and Radhakrishnan, V.: 1980, submitted to Astrophys. J.Google Scholar
Taylor, J.H. and Manchester, R.N.: 1975, Astron. J. 80, pp. 794–806.CrossRefGoogle Scholar
Taylor, J.H., Fowler, L.A., and McCulloch, P.M.: 1979, Nature 277, pp. 437–450.Google Scholar