Simulations of galaxy mergers Thorsten Naab MPA, Garching Evolution of galaxies, their central black holes and their large scale environment Potsdam, September,
The main growth modes of disks, bulges, and central black holes: Mergers - Violent Instabilities - Secular Evolution Frédéric Bournaud - CEA Saclay with.
Angular Momentum and the Formation of Stars and Black Holes Richard B. Larson Yale University.
Active Galaxies And Quasars![1]
The first hyper_luminous_infrared_galaxy_discovered_by_wise
17 Nov 2005 E.M. Sadler 1 SUMSS: The Sydney University Molonglo Sky Survey, 1997-2005.
The Galactic Centre: a hidden treasure How can we study the Galactic centre? How can we study the Galactic centre? What is do we find there? What is do.
Island Universes: Structure and Evolution of Disk Galaxies
The merging history of dark halos dominates galaxy formation. Spiral galaxies: merging of small, gas-rich substructures. Elliptical Galaxies: merging of.
The Powerful Black Hole Wind in the Luminous Quasar PDS 456
SUMSS: The Sydney University Molonglo Sky Survey, 1997-2005
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