Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-07T15:06:21.776Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio, optical and X-ray emission from pulsars

Published online by Cambridge University Press:  14 August 2015

B. Bertotti ,
A. Cavaliere  and
F. Pacini
B. Bertotti
Affiliation:
European Space Research Institute (ESRIN), Frascati, Rome
A. Cavaliere
Affiliation:
Laboratorio Gas Ionizzati (EURATOM-CNEN), Frascati, Rome
F. Pacini
Affiliation:
Laboratorio di Astrofisica, Frascati, Rome

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 examine the electromagnetic spectrum of the Crab Nebula pulsar NP 0532. The present observations are in rough agreement with the idea that the orbit of the radiating particles involves two different radii of curvature. One of the possible models requires electrons with a typical energy of the order of 100 MeV and a density ≈ 109 cm−3. A correlation length of about 10 cm could then give the coherence of the radio emission. Slow pulsars are unlikely to emit an appreciable amount of optical or X-ray radiation but a weak infrared emission is possible.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 196 - 201
Copyright
Copyright © Reidel 1970 

References

Bertotti, B., Cavaliere, A., and Pacini, F.: 1969a, Nature 221, 624.Google Scholar
Bertotti, B., Cavaliere, A., and Pacini, F.: 1969b, Nature 223, 1351.Google Scholar
Bradt, H., Rappaport, S., Mayer, W., Nather, F. H., Warner, B., Macfarlane, M., and Kristian, J.: 1969, Nature 222, 728.Google Scholar
Cavaliere, A.: 1969, ‘Emission Processes in Plasma’, paper given at the Pisa Meeting on Pulsars, 14–16 April.Google Scholar
Clark, R. R. and Smith, F. G.: 1969, Nature 221, 724.Google Scholar
Cocconi, G.: 1969, preprint.Google Scholar
Cocke, W. J., Disney, M. J., and Taylor, D. J.: 1969, Nature 221, 525.Google Scholar
Comella, J. M., Craft, H. D., Lovelace, R. V., and Sutton, J. M.: 1969, Nature 221, 453.Google Scholar
Finzi, A. and Wolf, R. A.: 1969, Astrophys. J. 155, L107.Google Scholar
Fritz, G., Henry, R. C., Meekins, J. F., Chubb, T. A., and Friedman, H.: 1969, Science 164, 709.Google Scholar
Ginzburg, V. L. and Syrovatskii, S. I.: 1965, Ann. Rev. Astron. Astrophys. 3, 297.Google Scholar
Ginzburg, V. L. and Syrovatskii, S. I.: 1969, Ann. Rev. Astron. Astrophys. 7, 375.Google Scholar
Ginzburg, V. L., Zhelezniakov, V. V., and Zaitsev, V. V.: 1968, Nature 220, 535.Google Scholar
Ginzburg, V. L., Zhelezniakov, V. V., and Zaitsev, V. V.: 1969, Astrophys. Space Sci. 4, 464.Google Scholar
Gold, T.: 1968, Nature 218, 731.Google Scholar
Gold, T.: 1969, Nature 221, 25.Google Scholar
Goldreich, P. and Julian, W. H.: 1969, Astrophys. J. 157, 869.Google Scholar
Gunn, J. F. and Ostriker, J. P.: 1969a, Nature 221, 454.Google Scholar
Gunn, J. F. and Ostriker, J. P.: 1969b, Phys. Rev. Letters 22, 728.Google Scholar
Haymes, R. C., Freeman, K. C., and Harnden, F. R. Jr.: 1969, Astrophys. J. 156, L107.Google Scholar
Michel, F. C.: 1969, Phys. Rev. Letters 23, 247.Google Scholar
Michel, F. C. and Tucker, W. H.: 1969, Nature 223, 277.Google Scholar
Pacini, F.: 1967, Nature 216, 567.Google Scholar
Pacini, F.: 1968, Nature 219, 145.Google Scholar
Radhakrishnan, V. and Cooke, D. J.: 1969, Astrophys. Letters 3, 225.Google Scholar