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Spatially-resolved X-ray spectroscopy of the core of the Centaurus cluster

By A. C. Fabian

Abstract

The Centaurus cluster, Abell 3526, at a redshift z = 0.0104 (Lucey, Currie & Dickens 1986) is a nearby, X-ray bright galaxy cluster. Analysis of ASCA, and earlier data (e.g. Allen et al. 2001) indicates it hosts a cooling flow (see Fabian 1994 for a review) o

Year: 2001
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