X-ray Cavities and Cooling Flows

Details X-ray Cavities and Cooling Flows X-ray Cavities and Cooling Flows

2003-11-12

arxiv.org/abs/astro-ph/0311284v1

Astronomy and Astrophysics

Astrophysics

5 pages, talk at IAU 2003 JD10, to appear in Highlights of Astronomy, vol. 13, ed. O. Engvold, IAU, 2003

Scientific paper

Recent data have radically altered the X-ray perspective on cooling flow clusters. X-ray spectra show that very little of the hot intracluster medium is cooler than about 1 keV, despite having short cooling times. In an increasing number of cooling flow clusters, the lobes of a central radio source are found to have created cavities in the hot gas. Generally, the cavities are not overpressured relative to the intracluster gas, but act as buoyant bubbles of radio emitting plasma that drive circulation as they rise, mixing and heating the intracluster gas. All this points to the radio source, i.e. an active galactic nucleus, as the heat source that prevents gas from cooling to low temperatures. However, heating due to bubbles alone seems to be insufficient, so the energetics of cooling flows remain obscure. We briefly review the data and theory supporting this view and discuss the energetics of cooling flows.

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