Antimatter in the Universe and the PAMELA/FERMI/AMS… anomaly Gerry Skinner [email protected] Max-Planck Institut fur Extraterrestriche Physik,
1 Nomenclature revisited No more than 5 mins or so on this From yesterday and subsequent feedback it is clear that many here are: From yesterday and subsequent.
1 Module 8: Clusters of Galaxies. General properties, masses and mass-to-light ratios, galaxy interactions, dynamic stability, the inter-galactic medium,
Physics 133: Extragalactic Astronomy and Cosmology Lecture 10; February 12 2014.
The Pierre Auger Observatory & Ultra High Energy Cosmic Rays Nick Cowan UW Astronomy January 2006.
Probing dark matter clustering using the Lyman- forest Pat McDonald (CITA) COSMO06, Sep. 28, 2006.
Galaxies Sylvain Veilleux My Interests: Galaxy and black hole formation and evolution Origin of starburst and AGN activity Role of galaxy mergers.
Active Galactic Nuclei (or AGN) Seyfert galaxies have very small (unresolved), extremely powerful centers! The strength of the emission lines vary on timescales.
High-resolution X-ray spectroscopy with microcalorimeters L. Piro Some key scientific drivers: –GRB engine and progenitors: X-ray lines and absorption.
24-Jun-2008K. Sembach 1 What’s Happening During Hubble Servicing Mission 4? Ken Sembach STScI Hubble Project Scientist.
Probing inflation, dark matter, dark energy, etc. using the Lyman- forest Pat McDonald (CITA) Collaborators: Uros Seljak, Anze Slosar, Alexey Makarov,
Galaxies with extremely violent energy release in their nuclei Active Galactic Nuclei (AGN) Up to many thousand times more luminous than the entire.
