Astrophysical radiation magnetohydrodynamics: Applications

Thomas J. Bogdan


The theory of radiation magnetohydrodynamics developed in the first lecture will now be applied to astrophysical problems of interest, namely: radiatively driven wind driving and accretion, and turbulent magnetic dynamos including radiative transfer.

Date: Mercredi, le 10 octobre 2018
Heure: 13:30
Lieu: Université de Montréal
  Pavillon Roger-Gaudry, Local D-460
Contact: Paul Charbonneau