Abstract
THE radio astronomy station of the P. N. Lebedev Physical Institute of the USSR Academy of Sciences in Pushchino (near Serpukhov) is investigating pulsars in the metre wavelength range. The east–west arm of the cross radio telescope DCR-1000 is used, and we can observe a pulsar for about 1 min each day.
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 SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
VITKEVICH, V., ALEKSEEV, Y., ZHURAVLEV, V. et al. Pulsar PP 0943. Nature 224, 49 (1969). https://doi.org/10.1038/224049a0
Received:
Issue date:
DOI: https://doi.org/10.1038/224049a0
This article is cited by
-
Individual and integrated pulse properties of PSR B0943+10 involved in the mode-changing phenomenon
Journal of Astrophysics and Astronomy (1998)
-
Pulsars. Survey of observational data
Astrophysics (1980)
-
Timing results for thirteen pulsars
Nature (1974)
-
Observations of PP 0943
Nature (1970)
