Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, H15(5), p. 279-279, 2009
DOI: 10.1017/s1743921310009221
Links
Tools
Cool gas in brightest cluster galaxies
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
Published version:
archiving forbidden
Data provided by 
Abstract
AbstractGas in galaxy clusters requires re-heating. We study the re-heating of the cool gas phases. Ionized and molecular gas is traced out to 20 kpc and found to be strongly coupled. The observed line emission may in part be explained by excitation due to hot, young stars.
