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Quantifying “Feedback” in Cool Core and Non-Cool Core Clusters

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Heating versus Cooling in Galaxies and Clusters of Galaxies

Part of the book series: Eso Astrophysics Symposia ((ESO))

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Author information

Authors and Affiliations

  1. Department of Physics, University of Durham, Durham, DH1 3L3, United Kingdom

    I. G. McCarthy & R. G. Bower

  2. Department of Physics and Astronomy, University of Victoria, Victoria, BC,V8P 5C2, Canada

    A. Babul

  3. Department of Physics and Astronomy, University of Waterloo, Waterloo, ON,N2L 5L4, Canada

    M. L. Balogh

Authors
  1. I. G. McCarthy
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  2. A. Babul
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  3. R. G. Bower
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  4. M. L. Balogh
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Editor information

Editors and Affiliations

  1. Max-Planck-Institut, für extraterrestrische Physik, Giessenbachstraβe, 85748 Garching, Germany

    H. Böhringer , G.W. Pratt , A. Finoguenov  & P. Schuecker , ,  & 

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© 2007 Springer-Verlag Berlin Heidelberg

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McCarthy, I.G., Babul, A., Bower, R.G., Balogh, M.L. (2007). Quantifying “Feedback” in Cool Core and Non-Cool Core Clusters. In: Böhringer, H., Pratt, G., Finoguenov, A., Schuecker, P. (eds) Heating versus Cooling in Galaxies and Clusters of Galaxies. Eso Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-73484-0_41

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