Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-02T21:38:29.250Z Has data issue: false hasContentIssue false
  • English
  • Français

Color Maps of A 1795 and A 2597 - Cooling Flow Cluster Central Galaxies with Active Nuclei

Published online by Cambridge University Press:  07 August 2017

W. Romanishin
W. Romanishin*
Affiliation:
Physics Department, Arizona State University, Tempe, AZ 85287-1504

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The subject of cooling flows in clusters of galaxies remains a controversial one, primarily because many clusters which have large x-ray derived mass inflow rates do not show any optical manifestation of the inflow or of the final fate of the gas. However, a handful of cooling flow clusters do show extended blue continuum regions indicative of current star formation which may be caused by the cooling flows (Romanishin 1987, Romanishin and Hintzen 1988), while another group show spectral evidence of star formation (O'Connell and McNamara 1988). Most of the cluster galaxies which show evidence of star formation also show nuclear activity, in the form of radio emission.

Type
Part 8: Relationships of Nucleus, Galaxy and Environment
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 460 - 461
Copyright
Copyright © Kluwer 1989 

References

Antonucci, R. R. J. 1985, Ap. J. Suppl., 59, 499.Google Scholar
Johnstone, R. M., Fabian, A. C., and Nulsen, P. E. J. 1987, M.N.R.A.S. 224, 75.Google Scholar
O'Connell, R. W., and McNamara, B. R. 1988 in Cooling Flows in Clusters and Galaxies ed. Fabian, A. C. (Dordrecht:Kluwer), p. 103.CrossRefGoogle Scholar
Romanishin, W. 1987. Ap.J. (Letters), 323, L113.Google Scholar
Romanishin, W., and Hintzen, P. 1987. Ap.J. (Letters) 324, L17.Google Scholar
van Breugel, W. J. M., Heckman, T., and Miley, G. 1984. Ap.J. 276, 79.Google Scholar