Thermal Conduction in Clusters of Galaxies

Abstract

We estimate the thermal conductivity of a weakly collisional magnetized plasma with chaotic magnetic field fluctuations. When the fluctuation spectrum extends over two or more decades in wave-vector, we find that thermal conduction is very efficient; the conduction coefficient is only a factor ~5 below the classical Spitzer estimate. We suggest that conduction could play a significant role in cooling flows in clusters of galaxies.

4 pages, 2 figures. Accepted for publication in ApJ Letters

References in corpus (3)

• Is the gas in cooling-flows multi-phase?
• XMM-Newton observations of M87 and Its X-Ray Halo
• Chandra X-ray observations of the 3C295 cluster core

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