Abstract
Stars with a dipole magnetic field oriented at an angle to the rotation axis may emit pulsating radio signals.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Maran, S. P., and Cameron, A. G. W., Physics Today (August 1968).
Pacini, F., Nature, 219, 145 (1968).
Ostriker, J., Nature, 217, 1227 (1968).
Ledoux, P., and Renson, P., Ann. Rev. Astron. Astrophys. (1966).
Gold, T., Nature, 218, 731 (1968).
Nodvick, J. S., and Saxon, D. S., Phys. Rev., 96, 180 (1954).
Bekefi, G., Radiation Processes in Plasma (John Wiley and Sons, New York, 1966).
Robinson, B. J., Cooper, B. F. C., and Gardiner, F. F., Nature, 218, 1143 (1968).
Westfold, K. C., Astrophys. J., 130, 241 (1959).
Oster, L., Phys. Rev., 119, 1444 (1960).
Craft, H. D., Comella, J. M., and Drake, F. D., Nature, 218, 1122 (1968).
Rickett, B. J., and Lyne, A. G., Nature, 218, 934 (1968).
Grueff, G., Roff, G., and Vigotti, M., Nature, 218, 1036 (1968).
Perkins, W. A., and Barr, W. L., Phys. Fluids, 11, 388 (1968).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
EASTLUND, B. Oblique Rotator and Pulsar Radiation. Nature 220, 1293–1296 (1968). https://doi.org/10.1038/2201293a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/2201293a0
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.