Abstract
PSR 1237 + 25 has a short-period subpulse system in which subpulses: march in a sense opposite to that found in other pulsars and a long-period system which is strongest in the midpulse region where the short-period system disappears.
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
Backer, D. C., Nature, 227, 692 (1970).
Lang, K. R., Astrophys. J. Lett., 161, L133 (1970).
Drake, F. D., and Craft, H. D., Nature, 220, 231 (1968).
Vitkevich, V. V., and Shitov, Yu. P., Nature, 225, 248 (1970).
Sutton, J. M., Staelin, D. H., Price, R. M., and Weimer, R., Astrophys. J. Lett., 159, L89 (1970).
Backer, D. C., Nature, 228, 42 (1970).
Komesaroff, M. M., Nature, 225, 612 (1970).
Manchester, R. N., Nature, 228, 264 (1970).
Sturrock, P. A., Nature, 227, 465 (1970).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
BACKER, D. Correlated Subpulse Structure in PSR 1237 + 25. Nature 228, 752–755 (1970). https://doi.org/10.1038/228752a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/228752a0
This article is cited by
-
A study of PSR1237 + 25 at 430 MHz
Nature (1980)
-
Drifting subpulses and pulsar slowdown rates
Nature (1975)
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.