Skip to main content
Log in

Observation of a Rapidly Pulsating Radio Source

  • Article
  • Published:

From Nature

View current issue Submit your manuscript

Unusual signals from pulsating radio sources have been recorded at the Mullard Radio Astronomy Observatory. The radiation seems to come from local objects within the galaxy, and may be associated with oscillations of white dwarf or neutron stars.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1.
Fig. 2.
Fig. 3.
Fig. 4.

Similar content being viewed by others

References

  1. Hewish, A., Scott, P. F., and Wills, D., Nature, 203, 1214 (1964).

    Article  ADS  Google Scholar 

  2. Cameron, A. G. W., Nature, 205, 787 (1965).

    Article  ADS  Google Scholar 

  3. Finzi, A., Phys. Rev. Lett., 15, 599 (1965).

    Article  ADS  Google Scholar 

  4. Meltzer, D. W., and Thorne, K. S., Ap. J., 145, 514 (1966).

    Article  ADS  Google Scholar 

  5. Greenstein, J. L., in Handbuch der Physik, L., 161 (1958).

    Google Scholar 

  6. Fichtel, C. E., and McDonald, F. B., in Annual Review of Astronomy and Astrophysics, 5, 351 (1967).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

HEWISH, A., BELL, S., PILKINGTON, J. et al. Observation of a Rapidly Pulsating Radio Source. Nature 217, 709–713 (1968). https://doi.org/10.1038/217709a0

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1038/217709a0

  • Springer Nature Limited

This article is cited by

Navigation