Facts about SNe and their remnants
Observational Probes of Dark Energy Timothy McKay University of Michigan Department of Physics Observational cosmology: parameters (H 0, 0 ) => evolution.
Stellar Feedback and Evolution of Milky Way-like Galaxies
Jon Morse PI (ASU), Chris Fryer (LANL), Robert Kirshner (Harvard), Tod R. Lauer (NOAO),
2005 Aspen Winter Conference The Highest Energies February 17, 2005
The SNAP Instrument Suite Session 126.04
SuperNova Acceleration Probe Research and Development Efforts
Facts about SNe and their remnants Evolution of an SNR sensitively depends on its environment. Observed SNRs are typically produced by SNe in relative.
X-ray study of a nearby nuclear X-ray study of a nearby nuclear starburst and a nearby AGN starburst and a nearby AGN Roberto Soria (UCL) Mat Page, Kinwah.
Astronomy and Astrophysics Advisory Committee Meeting NSF Headquarters; October 12, 2006
How Do Supermassive Black Holes Get Starved?
Yashar Akrami