Modelling the Atomic and Molecular Gas in Galaxies and Comparisons wih GASS and COLD GASS Results
14 Sep 2006NVO Summer School 20061 T HE US N ATIONAL V IRTUAL O BSERVATORY Shape of Galaxy Rotation Curves A multiwavelength study using the VO Barbara.
Less than 10% of star formation in z~0.6 massive galaxies is directly triggered by galaxy mergers Aday R. Robaina & Eric Bell, Ros Skelton, Dan McIntosh,
Galaxy groups Michael Balogh Department of Physics and Astronomy University of Waterloo.
Conference Introduction Duncan Forbes Swinburne University.
Current Topics: Lyman Break Galaxies - Lecture 5 Current Topics Lyman Break Galaxies Dr Elizabeth Stanway ([email protected])
Galaxies. Galactic Morphology Interacting Galaxies "Active" Galaxies.
Star-Forming Galaxies and the IGM in the z=1.5-2.5 Redshift Desert C. Steidel, D. Erb, N. Reddy (Caltech) A. Shapley (Berkeley) M. Pettini (IoA, Cambridge)
Simulations of galaxy mergers Thorsten Naab MPA, Garching Evolution of galaxies, their central black holes and their large scale environment Potsdam, September,
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?
High Redshift Galaxies in the Great Observatories Origins Deep Survey (GOODS) Mark Dickinson (National Optical Astronomy Observatory) for the GOODS team.
Candels the correlation_between_galaxy_morphology_and_star_formation_activity_at_z2
