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1 Introduction
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2 Spectroscopic evidence for the absence of low temperature
phases and local isothermality in cooling flow regions
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3 The interpretation of cooling flow spectra and cluster intrinsic
absorption
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4 Non-detection of sufficient internal absorption in two test cases
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5 Evidence for inhomogeneities and mass deposition in X-ray images
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6 Problems of cooling flows in rotating clusters
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7 Heating model
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8 Magnetic fields
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9 Conclusions
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Appendix A
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References
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