3560 y 3750X
Università di Roma Tor Vergata & INAF-IASF Roma [email protected].
Can a double component outflow explain the X-ray and Optical Lightcurves of GRBs? Massimiliano De Pasquale 1 P. Evans 2, S. Oates 1, M. Page 1, S. Zane.
Observational evidences of CR acceleration at shocks chung-ming ko institute of astronomy and department of physics, national central university, taiwan.
TeV blazars and their distance E. Prandini, Padova University & INFN G. Bonnoli, L. Maraschi, M. Mariotti and F. Tavecchio Cosmic Radiation Fields - Sources.
Chandra Monitoring of X-Ray Evolution of SNR 1987A
CIR Session Summary at Kennebunkport
The Universe >100 MeV Brenda Dingus Los Alamos National Laboratory.
Fermi LAT measurements of blazar spectra and implications on their structure
