Slide 1http://chandra.h arvard.edu/phot o/2007/m51/ Slide 2 Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies Q. Daniel Wang, Shikui…

Slide 1Galaxy Mergers: major/minor wet/dry Hans-Walter Rix MPIA, Heidelberg … which galaxies are most shaped by mergers? … when do mergers matter for the SFR? … inevitable…

Slide 1The Thick Disks of Spiral Galaxies as Relics from Gas-Rich, Turbulent, Clumpy Disks at High Redshifts Frédéric Bournaud, Bruce G. Elmegreen, and Marie Martig 2009,…

Slide 1 KASI Galaxy Evolution Journal Club Comparing the Relation between Star Formation and Galaxy Mass in Different Environments - B. Vulcani et al. 2010, ApJ, 710, L1…

Slide 1Cracking the mystery of galaxy and black hole formation: rachel somerville MPIA/STScI a Theorists’ Wish List for the next generation of Space Telescopes Slide 2…

Slide 1 Galactic Stellar Population Structure and kinematics Alessandro Spagna Osservatorio Astronomico di Torino 26 Febbraio 2002 Slide 2 Galactic Structure Flat disk: 10…

Slide 1 Weidong Li Jesse Leaman Alex Filippenko Department of Astronomy University of California, Berkeley Nearby Supernova Rates from the Lick Observatory Supernova Search…

Next Topic, Brute Force Let’s go measure a lot of redshifts, assume z tells us the distance, and see what we can see. => The “z machine of Huchra and Geller Velocity…

Galactic Stellar Population Structure and kinematics Alessandro Spagna Osservatorio Astronomico di Torino 26 Febbraio 2002 Galactic Structure Flat disk: 1011 stars (Pop.I)…

Next Topic, Brute Force Let’s go measure a lot of redshifts, assume z tells us the distance, and see what we can see. => The “z machine of Huchra and Geller Velocity…