A thermally stable heating mechanism for the intracluster medium: turbulence, magnetic fields and plasma instabilities Thermally stable heating of the ICM (2011)
Attributed to:
Turbulence, plasma instabilities, transport and magnetogenesis in galaxy clusters
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2010.17621.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2010.17621.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4