Galaxy Mergers: major/minor wet/dry Hans-Walter Rix MPIA, Heidelberg … which galaxies are most shaped by mergers? … when do mergers matter for the SFR?
Interpreting stellar populations in a cosmological context rachel somerville MPIA with thanks to the GOODS & GEMS teams, S. Faber, B. Allgood, J. Primack,
The Co-evolution of Galaxies and Dark Matter Halos Charlie Conroy (Princeton University) with Andrey Kravtsov, Risa Wechsler, Martin White, & Shirley Ho.
Fraction of galaxies of different types plotted as function of cluster radius and projected density Galaxy Morphology and Environment Main relation – E’s.
Active Galactic Nuclei Questions to be addressed: (1)What are active galactic nuclei (AGN)? (2) What are the main properties of AGN? (3) What is the source.
Open Questions Satellite galaxies II (and other stuff)
The Co-evolution of Galaxies and Dark Matter Halos
Galaxy Morphology and Environment Main relation – E’s more common in clusters than field
