Hostname: page-component-84b7d79bbc-lrf7s Total loading time: 0 Render date: 2024-07-29T23:49:26.332Z Has data issue: false hasContentIssue false
  • English
  • Français

Radiation from Pulsars

Published online by Cambridge University Press:  07 February 2017

I. Lerche
I. Lerche*
Affiliation:
Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Ill., U.S.A.

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 suggest that an oscillating interface, carrying a steady current between a rotating, radiating, magnetic dipole and an external plasma is the source of pulsar radiation produced over a broad band of high frequencies (108–1018 Hz). The efficiency of the radiation mechanism is so high that the oscillation energy goes mainly into radiation in each cycle of the oscillation.

Type
Session 8
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 449 - 454
Copyright
Copyright © Reidel 1971 

References

Bradt, H., Rappaport, S., Mayer, W., Nather, R. E., Warner, B., McFarlane, M., and Kristian, J.: 1969, Nature 222, 723.Google Scholar
Chiu, H.-Y.: 1970, The Crab Nebula Symposium, Flagstaff, Publ. Astron. Soc. Pacific 82, 487.Google Scholar
Gorenstein, P., Kellogg, E. M., and Gursky, H.: 1969, Astrophys. J. 156, 315.Google Scholar
Gunn, J. E. and Ostriker, J. P.: 1969, Nature 221, 454.Google Scholar
Lerche, I., 1970a, Astrophys. J. 159, 229.CrossRefGoogle Scholar
Lerche, I.: 1970b, Astrophys. J. 160, 1003.CrossRefGoogle Scholar
Lerche, I.: 1970c, Astrophys. J. 162, 153.Google Scholar
Maran, S. P. and Cameron, A. G. W.: 1969, ‘Progress Report on Pulsars’, first part of a report on the Fourth Texas Symposium on Relativistic Astrophysics, Dallas, Texas, December 1968.Google Scholar
Neugebauer, G., Becklin, E. E., Kristian, J., Leighton, R. B., Snellen, G., and Westphal, J. A.: 1969, Astrophys. J. 156, L115.Google Scholar
Oke, J. B.: 1969, Astrophys. J. 156, L49.Google Scholar
Pacini, F.: 1968, Nature 219, 145.Google Scholar