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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

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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