Can AGN and Radio Sources Reheat the Intracluster Medium?

De Young, D.S.; O’Neill, S. M.; Jones, T. W.

doi:10.1007/978-3-540-73484-0_36

D.S. De Young³,
S. M. O’Neill⁴ &
T. W. Jones⁴

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Authors and Affiliations

National Optical Astronomy Observatory, USA
D.S. De Young
Dept. of Astronomy, University of Minnesota, USA
S. M. O’Neill & T. W. Jones

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D.S. De Young
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S. M. O’Neill
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T. W. Jones
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Max-Planck-Institut, für extraterrestrische Physik, Giessenbachstraβe, 85748 Garching, Germany
H. Böhringer , G.W. Pratt , A. Finoguenov & P. Schuecker , , &

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De Young, D., O’Neill, S.M., Jones, T.W. (2007). Can AGN and Radio Sources Reheat the Intracluster Medium?. 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_36

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DOI: https://doi.org/10.1007/978-3-540-73484-0_36
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-73483-3
Online ISBN: 978-3-540-73484-0
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