Thermal Conduction in a Magnetized Hot Accretion Flows: A 2D Treatment in Viscouse-Resistive Regime

Details Thermal Conduction in a Magnetized Hot Accretion Flows: A 2D Treatment in Viscouse-Resistive Regime Thermal Conduction in a Magnetized Hot Accretion Flows: A 2D Treatment in Viscouse-Resistive Regime

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..427..102a&link_type=abstract

Accretion and Ejection in AGN: a Global View. Proceedings of a conference held June 22-26, 2009 in Como, Italy. Edited by Laura

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Scientific paper

Observations of the hot gas, which is surrounding Sgr A* and a few other nearby galactic nuclei, imply that mean free paths of electron and proton are comparable to gas capture radius. So, hot accretion flows likely proceed under week collision conditions. As a result thermal conduction by ions has a considerable contribution in transfer of the realized heat in accretion mechanisms. We have investigated the role of thermal conduction in a viscose-resistive accretion flow in a 2D treatment.

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