XMM-Newton Observations of the Perseus Cluster. I. The Temperature and Surface Brightness Structure

@article{Churazov2003XMMNewtonOO,
  title={XMM-Newton Observations of the Perseus Cluster. I. The Temperature and Surface Brightness Structure},
  author={Eugene Churazov and William R. Forman and C. Jones and Hans B{\"o}hringer},
  journal={The Astrophysical Journal},
  year={2003},
  volume={590},
  pages={225 - 237}
}
We present preliminary results of a XMM-Newton 50 ks observation of the Perseus Cluster that provides an unprecedented view of the central 0.5 Mpc region. The projected gas temperature declines smoothly by a factor of 2 from a maximum value of ~ 7 keV in the outer regions to just above 3 keV at the cluster center. Over this same range, the heavy-element abundance rises slowly from 0.4 to 0.5 solar as the radius decreases from 14' to 5', and then it rises to a peak of almost 0.7 solar at 1.′25… 

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