Abstract
AN optical jet, extending 10 arc min from the elliptical galaxy M89 (NGC4552) is reported here. Two low surface brightness shells partly surround the galaxy and a much fainter arc, 13 arc min away has also been detected. The jet was found on five deep plates of the Virgo cluster obtained by the 1.2-m UK Schmidt Telescope. Three sky-limited IIIaJ (bandpass 395–530 nm) and two IIIaF (630–685 nm) plates were taken on hypersensitised1 emulsions. A slightly different plate centre was used for two of the plates.
Similar content being viewed by others
References
Sim, M. E. Am. Astr. Soc. Phot. Bull. No. 14, 9–13 (1977).
Malin, D. F. Nature 276, 591–593 (1978).
Malin, D. F. Am. Astr. Soc. Phot. Bull. No. 16, 14–17 (1977).
Fraser, C. W. Astr. Astrophys. Suppl. 29, 161–194 (1977).
Heeschen, D. S. Astrophys. Lett. 6, 49–53 (1970).
Disney, M. J. & Cromwell, R. H. Astrophys. J. 164, L35–39 (1971).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
MALIN, D. A jet associated with M89. Nature 277, 279–280 (1979). https://doi.org/10.1038/277279a0
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/277279a0
- Springer Nature Limited
This article is cited by
-
Kinematical properties of early-type galaxies
The Astronomy and Astrophysics Review (1994)
-
Starbursts in the nuclei of shell galaxies
Nature (1992)
-
The off-focus photograph technique for low dispersion spectra
Astrophysics and Space Science (1990)