Hot Gas in Damped Lyman- Systems Hidden Baryons & Metals in Galactic Halos at z=2-4 Andrew Fox (ESO-Chile) with P. Petitjean, C. Ledoux, R. Srianand, J.
Bi-modality and Do w n s i z i n g Avishai Dekel HU Jerusalem Bernard ’ s Cosmic Stories, Valencia, June 2006 Origin of E vs S Galaxies.
In, Out, and Around: An Overview from Simulations David Weinberg, Ohio State University Collaborators: Amanda Brady Ford, Romeel Davé, Mark Fardal, Neal.
The coordinated growth of stars, haloes and large-scale structure since z=1 Michael Balogh Department of Physics and Astronomy University of Waterloo.
Kinemetry of High-Redshift Galaxies
The coordinated growth of stars, haloes and large-scale structure since z=1
Cool Halo Gas in a Cosmological Context
Cool Halo Gas in a Cosmological Context Kyle Stewart “Team Irvine” UC Santa Cruz Galaxy Formation Workshop 8-20-09 Kyle Stewart “Team Irvine” UC Santa.
1 Carlo Nipoti Dipartimento di Astronomia Università di Bologna Thermal evaporation, AGN feedback and quenched star formation in massive galaxies Chandra.
Driving Downsizing with groups of galaxies Michael Balogh Department of Physics and Astronomy University of Waterloo.
Genzel et al. 2008, astro-ph 0807.1184, Genel et al. astro-ph 0808.0194
The important role of galaxy groups
