Abstract.
The gas temperature in the cores of many clusters of galaxies drops inward by about a factor of three or more within the central 100 kpc radius. The radiative cooling time drops over the same region from 5 or more Gyr down to about 108yr. Although it would seem that cooling has taken place, XMM and Chandra spectra show no evidence for strong mass cooling rates of gas below 1-2 keV. Chandra images show holes coincident with radio lobes and cold fronts indicating that the core regions are complex. The observational situation is reviewed here and ways in which continued cooling may be hidden are discussed, together with the implications for any heat source which balances radiative cooling.
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Fabian, A.C. Cooling Flows in Clusters of Galaxies. In: Gilfanov, M., Sunyeav, R., Churazov, E. (eds) Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10856495_3
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DOI: https://doi.org/10.1007/10856495_3
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-43769-7
Online ISBN: 978-3-540-48014-3
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