1 Black Holes in the Early Universe Accretion and Feedback Geoff Bicknell & Alex Wagner Research School of Astronomy & Astrophysics Australian National.
A bit of (my) history My main PhD simulations were performed on COSMOS Mk I in 1998-99! My main PhD simulations were performed on COSMOS Mk I in 1998-99!
Galaxy Formation and Evolution, Mo, van den Bosch & White, 2010 Galactic Dynamics, Binney & Tremaine 2008.
Sravani Vaddi 1, Chris O’Dea 1, Stefi Baum 1, Christine Jones 2, Bill Forman2, Samantha Whitmore 3 and Rabeea Ahmed 3 1 Astrophysical Sciences & Technology,
The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051 Nick Devereux (ERAU) Emily Heaton (ERAU) May 22 nd, 2013 Naples, Italy.
COSPAR Workshop, Udaipur 2003 Active Galactic Nuclei : I Keith Arnaud NASA Goddard University of Maryland.
Ben Maughan (CfA)Chandra Fellows Symposium 2006 The cluster scaling relations observed by Chandra C. Jones, W. Forman, L. Van Speybroeck.
The Galactic Center is a Treasure Box of High Energy Physics The Nearest AGN and Star Burst Galaxy. I will report a current picture of the Galactic Center,
Feedback & Large Surveys Harry Ferguson (STScI). Feedback Behroozi+ 2011 Halo quenching Quasar mode AGN Radio Mode AGN (SNe) SNe Satellites: Ram pressure,
Andrii Elyiv and XMM-LSS collaboration
The Galactic Center is a Treasure Box of High Energy Physics
Supernovae and Masers in Arp220: Pushing the limits of VLBI sensitivity Supernovae and Masers in Arp220: Pushing the limits of VLBI sensitivity P.J.Diamond.