Abstract
MARKARYAN1 and Markaryan and Lipovetsky2 have given data on a few hundred galaxies with strong ultraviolet continua. Markaryan classifies them on the basis of the concentration of the source of the continuum (s means concentrated and d diffuse objects; sd and ds are intermediate). Especially among the s-type objects there seems to be contamination with QSOs when their spectra, colour and presumable morphology (spheroidal, compact) are considered. Redshifts are now available for many Markaryan galaxies providing new material for studies of the redshift problem. It is worthwhile to see whether the claimed peculiarities in redshifts of QSOs and related emission-line objects3–6 have counterparts in the distribution of these smaller redshifts. According to Arp and Sulentic (see ref. 7) many Markaryan galaxies seem to be companions of smallredshift bright galaxies and thus they possibly have anomalous redshifts.
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
Markaryan, B. E., Astrofizika, 3, 55–68 (1967); 5, 443–459, 581–592 (1969).
Markaryan, B. E., and Lipovetsky, V. A., Astrofizika, 7, 511–519 (1971); 8, 155–164 (1972).
Burbidge, G., Astrophys. J. Lett., 154, L41–48 (1968).
Karlsson, K. G., Nature phys. Sci., 245, 68–70 (1973).
Burbidge, G. R., and O'Dell, S. L., Astrophys. J., 178, 583–605 (1972).
Burbidge, G. R., and O'Dell, S. L., Astrophys. J. Lett., 186, L59–L62 (1973).
Arp, H., in Proc. I.A.U. Symp., 58 (in the press).
Weedman, D. W., and Khachikyan, E. E., Astrofizika, 4, 587–593 (1968); 5, 113–122 (1969).
Arakelyan, M. A., Dibai, E. A., and Esipov, V. F., Astrofizika, 6, 39–47 (1970); 8, 33–42, 177–186, 329–335 (1972).
Arakelyan, M. A., Dibai, E. A., Esipov, V. F., and Markaryan, B. E., Astrofizika, 6, 357–366 (1970); 7, 177–187 (1971).
Denisjuk, E. K., Astron. Tsirk., No. 621, 7–8 (1971); No. 624, 1–2 (1971); No. 759, 6–8 (1973).
Kopylov, I. M., Lipovetsky, V. A., Pronik, V. I., and Chuvaev, K. K., Astron. Tsirk., No. 755, 1–3 (1973).
Ulrich, M-M., J., Astrophys. J., 163, 441–447 (1971).
Sargent, W. L. W., Astrophys. J., 159, 765–772 (1970); 173, 7–24 (1972).
Sargent, W. L. W., and Huchra, J., Astrophys. J., 186, 433–443 (1973).
Rubin, V. C., Ford, W. K., jun., and Rubin, J. S., Astrophys. J. Lett., 183, L111–L115 (1973).
Arp, H., Astrophys. J., 185, 797–808 (1973).
Pecker, J. C., Tait, W., and Vigier, J. P., Nature, 241, 338–339 (1973).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
TEERIKORPI, P. Redshifts of Markaryan galaxies. Nature 252, 110–111 (1974). https://doi.org/10.1038/252110a0
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1038/252110a0
This article is cited by
-
Redshifts of compact galaxies in systems of galaxies
Astrophysics and Space Science (1977)
-
Quasars and the cosmological distance scale
Nature (1976)
-
Normal redshifts in Markaryan galaxies
Nature (1975)
-
Normal redshifts in Markaryan galaxies (reply)
Nature (1975)
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.