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Brightest Cluster Galaxies & Cooling Flows

Published online by Cambridge University Press:  21 March 2013

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

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