High energy emission from supernova remnants and regions of star formation Diego F. Torres [email protected] Lawrence Livermore Lab. California,
7/26/12W. Majid1 Crab Giant Pulses W. Majid *, S. Ellingson (PI), C. Garcia-Miro, T. Kuiper, J. Lazio, S. Lowe, C. Naudet, D. Thompson, K. Wagstaff * Jet.
July 4, 2006 P. Padovani, Unidentified -ray Sources 1 The Blazar Sequence: Validity and Predictions Paolo Padovani (ESO) Blazar properties The Blazar.
The Highest Energy Emission from Short Gamma-Ray Bursts Pablo Saz Parkinson Santa Cruz Institute for Particle Physics, UCSC SCIPP Seminar, 9 March 2007.
Jordan Goodman HAWC Review - December 2007 Education and Outreach Jordan A. Goodman University of Maryland.
HAWC: A Next Generation All-Sky VHE Gamma-Ray Telescope.
Jamie Holder VERITAS Collaboration Bartol Research Institute/ University of Delaware LS I +61° 303: The High Energy View "Getting Involved with GLAST"
Introduction A pulsar magnetosphere can be divided into two zones: The closed zone filled with a dense plasma co-rotating with the neutron star (NS), and.
Exploring the Gamma-Ray/Optical Connection in Blazars
High energy emission in Gamma Ray Bursts
High energy emission in Gamma Ray Bursts Gabriele Ghisellini INAF – Osservatorio Astronomico di Brera.
Statistical analysis of model-fitted inner-jets of the MOJAVE blazars Xiang Liu, Ligong Mi, et al. Xinjiang Astronomical Observatory (Former Urumqi Observatory),