Effervescent heating: constraints from nearby cooling flow clusters observed with XMM-Newton

2006/02/28 by R. Piffaretti, Rocco Piffaretti, Jelle Kaastra +1 · 9 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Star Formation Studies #Cooling flow #Flow (mathematics) #Galaxies: Formation, Evolution, Phenomena #Mechanics #Physics #Sample (material) #Solar and Space Plasma Dynamics #Thermodynamics #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054365

published in Astronomy and Astrophysics 453(2), 423-431 (EDP Sciences) · Final version accepted for publication in A&A. Conclusions on effervescent heating model changed

arxiv created 2006/05/15 · openalex publication_date 2006/06/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We have used deprojected radial density and temperature profiles of a sample of 16 nearby CF clusters observed with XMM-Newton to test whether the effervescent heating model can satisfactorily explain the dynamics of CF clusters.

Citations

• ChandraObservations of the Central Region of A3112
• ChandraObservation of the Central Region of the Cooling Flow Cluster A262: A Radio Source That Is a Shadow of Its Former Self?
• The X-ray virial relations for relaxed lensing clusters observed withChandra
• Strong Turbulence in the Cool Cores of Galaxy Clusters: Can Tsunamis Solve the Cooling Flow Problem?
• Deep inside the core of Abell 1795: theChandraview
• Magnetic Field in Clusters of Galaxies