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Brightest Cluster Galaxies & Cooling Flows.
- Source :
- Proceedings of the International Astronomical Union; Aug2012 Supplement, Vol. 8 Issue S292, p169-174, 6p
- Publication Year :
- 2012
-
Abstract
- 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. [ABSTRACT FROM PUBLISHER]
Details
- Language :
- English
- ISSN :
- 17439213
- Volume :
- 8
- Issue :
- S292
- Database :
- Complementary Index
- Journal :
- Proceedings of the International Astronomical Union
- Publication Type :
- Academic Journal
- Accession number :
- 87364930
- Full Text :
- https://doi.org/10.1017/S1743921313000975