1. The Chemical Evolution of the Galaxy and Dwarf Spheroidals of the Local Group Saas-Fee, March 4-10, 2007 2. Chemical Evolution of the Galaxy and dSphs of the Local Group…
Slide 1Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, [email protected] 1 Aldo Morselli INFN, Sezione di Roma 2 & Università…
Slide 1 The Pierre Auger Observatory & Ultra High Energy Cosmic Rays Nick Cowan UW Astronomy January 2006 Slide 2 Outline What are UHECRs? How are they produced? Why…
Spectral Analysis and Galaxy Properties Tinggui Wang USTC, Hefei What can a galaxy spectrum tell? 3 components star-light, emission lines, occasionally, interstellar absorption…
Hot Gas and Outflows of Nearby Normal Galaxies Q. Daniel Wang (UMass) Most of present galaxies are not nuclear starbursters Phenomena that would be otherwise overwhelmed…
Feedback: in the form of outflow AGN driven outflow M82 Blue: Chandra Red: Spitzer Cyan: Optical Star formation driven outflow Two categories of the gas in a SF/SB galaxy…
Diffuse Gamma Rays: A Model-Independent Approach by Tijana Prodanović Brian D. Fields University of Illinois at Urbana-Champaign Outline Use model-independent ways of constraining…