Radiatively inefficient accretion disks
Abstract
Description
Radiatively inefficient (or advection dominated) disks are discussed at an introductory level. Ion supported and radiation supported flows are discussed, the different consequences of advection dominated flows onto black holes vs. solid surfaces (neutron stars, white dwarfs), hydrodynamics, the role of the ratio of specific heats, and the possible connection between ADAFs and outflows.
To appear in: The neutron star black hole connection (NATO ASI ELOUNDA 1999) ed. C. Kouveliotou et al. New version: typos and other corrections
To appear in: The neutron star black hole connection (NATO ASI ELOUNDA 1999) ed. C. Kouveliotou et al. New version: typos and other corrections