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Cold Gas in Cluster Cores

  • Conference paper
Heating versus Cooling in Galaxies and Clusters of Galaxies

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

Summary

I review the literature’s census of the cold gas in clusters of galaxies. Cold gas here is defined as the gas that is cooler than X-ray emitting temperatures (∼ 107K) and is not in stars. I present new Spitzer IRAC and MIPS observations of Abell 2597 that reveal significant amounts of warm dust and star formation at the level of 5 solar masses per year.

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Author information

Authors and Affiliations

  1. Physics & Astronomy Dept, Michigan State University, East Lansing, MI US 48824-2320

    M. Donahue

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  1. M. Donahue
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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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Donahue, M. (2007). Cold Gas in Cluster Cores. 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_3

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