Abstract
High-frequency measurements suggest that the spectrum of the pulsating radio source is extremely steep.
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).
Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
MOFFET, A., EKERS, R. Detection of the Pulsed Radio Source CP 1919 at 13 cm Wavelength. Nature 218, 227–229 (1968). https://doi.org/10.1038/218227a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/218227a0
This article is cited by
-
Detection of Six Pulsars at 2.8 cm
Nature Physical Science (1972)
-
Average Pulsar Energies at Centimetre Wavelengths
Nature (1969)
-
Evidence in Support of a Rotational Model for the Pulsar PSR 0833–45
Nature (1969)
-
Pulsare, eine neue Klasse radioastronomischer Objekte
Die Naturwissenschaften (1969)
-
Pulsed Radio Sources
Nature (1968)
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.