Abstract
THE purpose of this letter is to draw attention to the very high redshift, z = 3.40, of the QSO OH471.
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
Gearhart, M. J., Lund, J. M., Frantz, D. J., and Kraus, J. P., Astrophys. J. 77, 557 (1972).
Lynds, R., and Wills, D., Nature 226, 532 (1970).
Lynds, R., Astrophys. J. Lett. 164, L73 (1971).
McCrea, W. H., Publ. Astron. Soc. Pacific, 78, 49 (1966).
Strittmatter, P. A., and Burbidge, G. R., Astrophys J. 147, 13 (1967).
Bahcall, J. N., and Sargent, W. L. W., Astrophys J. Lett. 148, L65 (1967).
Browne, I. W. A., and McEwan, N. J., Nature Physical Science 239, 101 (1972).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
CARSWELL, R., STRITTMATTER, P. Redshift of OH471. Nature 242, 394–395 (1973). https://doi.org/10.1038/242394a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/242394a0
This article is cited by
-
On the optical observation of galaxies with large redshifts
Nature (1977)
-
Prediction of radio structure in the two largest redshift QSOs
Nature (1974)
-
Radio spectra of OH471 and OQ172
Nature (1974)
-
Photoelectric photometry of OH471 and OQ172, and other optical objects near radio sources
Nature (1974)
-
Radio source identified with a neutral stellar object near an unusual galaxy
Nature (1974)
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.