Abstract
For the spectral determination of the temperature distribution in galaxy clusters we developed a double background subtraction method, and applied it to 2 morphology unbiased samples of X-ray luminous galaxy clusters (12 at z ∼0.2, 13 at z ∼0.3) observed by XMM-Newton. The scaled profiles of the X-ray properties show a self-similar behaviour above 0.2r500 for both samples. The tight X-ray scaling relations of the 2 samples show no evolution compared to the nearby and more distant samples. The X-ray lensing masses converge for most clusters.
Original language | English |
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Title of host publication | Heating versus Cooling in Galaxies and Clusters of Galaxies |
Subtitle of host publication | Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference held in Garching, Germany, 6-11 August 2006 |
Editors | Hans Böhringer , Gabriel W. Pratt , Alexis Finoguenov , Peter Schuecker |
Publisher | Springer |
Pages | 60-62 |
Number of pages | 3 |
ISBN (Electronic) | 978-3-540-73484-0 |
ISBN (Print) | 978-3-540-73483-3 |
DOIs | |
Publication status | Published - 2007 |
Event | MPA/ESO/MPE/USM Joint Astronomy Conference - Garching, Germany Duration: 6 Aug 2006 → 11 Aug 2006 Conference number: C06-08-06.1 |
Publication series
Name | Eso Astrophysics Symposia |
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Conference
Conference | MPA/ESO/MPE/USM Joint Astronomy Conference |
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Abbreviated title | COOL 06 |
Country/Territory | Germany |
City | Garching |
Period | 6/08/06 → 11/08/06 |