Outflows, Accretion Disks & the IGM: High Resolution
Chandra & XMM Spectroscopy of AGN
*Tahir Yaqoob, B. McKernan, U. Padmanabhan,
P. Serlemitsos, I. George, J. Turner, J. Reeves
*Johns Hopkins University
3400 N. Charles St.
Baltimore, MD 21218
We discuss the principal new results which have emerged from
over five years of high resolution X-ray spectroscopy of Active
Galactic Nuclei with Chandra and XMM. The picture emerging from
measurments of absorption and emission lines, both from the soft
X-ray band and the Fe K band is one which is more complex than
anticipated during the ASCA era and provides important new clues
on the dynamics and physical state of circumnuclear matter, as
well as the putative accretion disk, and in some cases the IGM.
The current data provide a tantalizing glimpse into an even richer
phenomenology which will likely be uncovered by Astro-E2 and
future missions. We show some simulations illustrating how Astro-E2
will resolve some key dengeneracies in the cuurent data and therefore
provide unique constraints on the ionization structure and kinematics
of matter in the central engine of AGN.