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astro-ph2003
Interaction of the AGN and X-ray Emitting Gas
Paul Nulsen
The process that prevents the deposition of cooled gas in cooling flows must rely on feedback in order to maintain gas with short cooling times, while preventing the bulk of the ga…
astro-ph2003★ 10 cited
Uniformity of foreground Galactic neutral Hydrogen over cooling flow clusters
David G. Barnes, Paul E. J. Nulsen
Radio maps at 21 cm of foreground neutral hydrogen over three cooling flow clusters of galaxies show that the foreground gas is uniform on scales from about 1 -- 10 arcmin. Five si…