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Heating rate profiles in galaxy clusters

Heating rate profiles in galaxy clusters
Heating rate profiles in galaxy clusters
The results of hydrodynamic simulations of the Virgo and Perseus clusters suggest that thermal conduction is not responsible for the observed temperature and density profiles. As a result it seems that thermal conduction occurs at a much lower level than the Spitzer value. Comparing cavity enthalpies to the radiative losses within the cooling radius for seven clusters suggests that some clusters are probably heated by sporadic, but extremely powerful, AGN outflows interspersed between more frequent but lower power outflows.
9783540734833
251-256
Springer
Pope, E.C.D.
8ce8f103-b1ba-4a35-ad78-1d968abe1bb5
Pavlovski, G.
6acbdaa4-3c28-4287-864d-77649b93959c
Kaiser, C.R.
a486973d-799c-401e-aa99-47dddd3972f7
Fangohr, H.
9b7cfab9-d5dc-45dc-947c-2eba5c81a160
Böhringer, H.
Pratt, G.W.
Finoguenov, A.
Schuecker, P.
Pope, E.C.D.
8ce8f103-b1ba-4a35-ad78-1d968abe1bb5
Pavlovski, G.
6acbdaa4-3c28-4287-864d-77649b93959c
Kaiser, C.R.
a486973d-799c-401e-aa99-47dddd3972f7
Fangohr, H.
9b7cfab9-d5dc-45dc-947c-2eba5c81a160
Böhringer, H.
Pratt, G.W.
Finoguenov, A.
Schuecker, P.

Pope, E.C.D., Pavlovski, G., Kaiser, C.R. and Fangohr, H. (2007) Heating rate profiles in galaxy clusters. Böhringer, H., Pratt, G.W., Finoguenov, A. and Schuecker, P. (eds.) In Heating versus Cooling in Galaxies and Clusters of Galaxies: Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006. vol. 2007, Springer. pp. 251-256 . (doi:10.1007/978-3-540-73484-0_46).

Record type: Conference or Workshop Item (Paper)

Abstract

The results of hydrodynamic simulations of the Virgo and Perseus clusters suggest that thermal conduction is not responsible for the observed temperature and density profiles. As a result it seems that thermal conduction occurs at a much lower level than the Spitzer value. Comparing cavity enthalpies to the radiative losses within the cooling radius for seven clusters suggests that some clusters are probably heated by sporadic, but extremely powerful, AGN outflows interspersed between more frequent but lower power outflows.

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Published date: 27 September 2007
Venue - Dates: MPA/ESO/MPE/USM Joint Astronomy Conference, Garching, Germany, 2006-08-06 - 2006-08-11

Identifiers

Local EPrints ID: 65054
URI: http://eprints.soton.ac.uk/id/eprint/65054
ISBN: 9783540734833
PURE UUID: 5a99f8b4-937f-408e-8027-1d65eee735d9
ORCID for H. Fangohr: ORCID iD orcid.org/0000-0001-5494-7193

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Date deposited: 29 Jan 2009
Last modified: 16 Mar 2024 03:09

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Contributors

Author: E.C.D. Pope
Author: G. Pavlovski
Author: C.R. Kaiser
Author: H. Fangohr ORCID iD
Editor: H. Böhringer
Editor: G.W. Pratt
Editor: A. Finoguenov
Editor: P. Schuecker

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