Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-19T08:42:54.203Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectroscopic Evidences for Star Formation in Cooling Flow Galaxies

Published online by Cambridge University Press:  25 May 2016

N. Cardiel ,
J. Gorgas  and
A. Aragon-Salamanca
N. Cardiel
Affiliation:
Dpto. de Astrofísica, Universidad Complutense, Madrid
J. Gorgas
Affiliation:
Dpto. de Astrofísica, Universidad Complutense, Madrid
A. Aragon-Salamanca
Affiliation:
Institute of Astronomy, Cambridge, UK

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.

X-ray observations have led to the conclusion that many galaxy clusters are hosting cooling flows. The brightest cluster galaxies could have accreted masses of the order of 1011–1012M⊙, but is still uncertain what the final fate of the accreted gas may be.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 349
Copyright
Copyright © Kluwer 1996