Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between.
The cosmological formation of massive galaxies Thorsten Naab MPA, Garching What regulates galaxy formation? Leiden, April, 22 nd.
Kelley Liebst AST 591 School of Earth and Space Exploration Arizona State University.
Massive galaxies at high redshift: models confront observations rachel somerville STScI rachel somerville STScI GIRLS; Leiden, September 2008.
The Evolution of Stars and Gas in Galaxies: PhD Midterm Philip Lah A journey with noise and astrometry.
Probing dark matter clustering using the Lyman- forest Pat McDonald (CITA) COSMO06, Sep. 28, 2006.
Neutral Hydrogen Gas in Star Forming Galaxies at z=0.24 Philip Lah Frank Briggs (ANU) Jayaram Chengalur (NCRA) Matthew Colless (AAO) Roberto De Propris.
