Image Details
Caption: Fig. 5.
Ratio of the mass accretion rate ﹩\dot{M}( r) ﹩ in models with heating by relativistic particles (αr = 2 × 10−4) and heat conduction to that in the nominal model (no heat conduction or heating by relativistic particles).
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.