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Mapping small-scale temperature and abundance structures in the core of the Perseus cluster

Monthly Notices of the Royal Astronomical Society, no. 3 (2004): 952-972

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We report further results from a 191-ks Chandra observation of the core of the Perseus cluster, Abell 426. The emission-weighted temperature and abundance structures are mapped in detail. There are temperature variations down to ∼1 kpc in the brightest regions. Globally, the strongest X-ray surface brightness features appear to be caused ...更多

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