Abstract
THE four rapidly pulsating radio sources discovered by Hewish et al.1 have been tentatively identified with neutron stars or white dwarfs, and their optical identification is therefore of great interest.
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
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968).
Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968).
Hewish, A., Meeting of the Royal Astronomical Society (London, April 10, 1968).
Johnson, H. L., Astrophys. J., 116, 640 (1952).
Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968).
Radhakrishnan, V., Komesaroff, M. M., and Cooke, D. J., Nature, 218, 229 (1968).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
JELLEY, J., WILLSTROP, R. Search for Optical Flashes from the Radio Source CP 1919. Nature 218, 753–755 (1968). https://doi.org/10.1038/218753a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/218753a0
This article is cited by
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.