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Brightest Cluster Galaxies & Cooling Flows

Published online by Cambridge University Press:  21 March 2013

Philippe Salomé
Philippe Salomé*
Affiliation:
LERMA, Observatoire de Paris 61 av. de l'Observatoire, F-75014 Paris, France email: philippe.salome@obspm.fr
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Abstract

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In the absence of any form of feedback heating, the gas in the central regions of massive relaxed cluster should cool and initiate a cooling flow. The presence/efficiency of an additional heating and the ultimate fate of the cooling gas is the subject of an extensive debate. In the last decade, molecular and atomic gas have been found in many Brightest Cluster Galaxies. I will review these observational results and discuss their implication for galaxy formation/evolution, in the perspective of ALMA.

Keywords

galaxies: cooling flows — intergalactic medium — galaxies: elliptical and lenticularcD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 169 - 174
Copyright
Copyright © International Astronomical Union 2013

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