I will summarize recent developments in modeling of mass outflows from
accretion disks in active galactic nuclei. I will discuss how
the hydrodynamical and magnetohydrodynamical wind structures revealed in
numerical simulations relate to observations. In particular,
I will present synthetic line profiles predicted by the simulations and
compare them with observations of broad line quasars.
Tuesday, November 30th
Seminar is to be held at 4:00 PM in the conference room
on the second floor of Dearborn Observatory
Refreshments will be served at 3:30
|
