Stephen C.-Y. Ng HKU. Outline What are pulsar wind nebulae? Physical properties and evolution Why study PWNe? Common TeV sources, particle accelerators.
Blazar Gamma-ray absorption by cosmic radiation fields GRB Fermi z~60-6 CTA Susumu Inoue (Kyoto University) with (more than) a little help from my friends.
Gamma-ray absorption by cosmic radiation fields
Joachim Isbert PAMELA 2009 Observations of High Energy Cosmic Ray Electrons by the ATIC Balloon Experiment 1.Louisiana State University, Department of.
Current Status of Physics & Future Prospect @ KEKB NP Higgs SM Figure by Dr. Hayasaka (Nagoya Univ.) June 20, 2007 Supersymmetry in 2010’s @ Hokkaido Univ.
Origin of the Cosmic Ray Positrons Observed Near Earth_1502.01244
Pulsar Wind Nebulae at High Energies
Dark Matter
J. Isbert Jefferson Lab 2009 Observations of High Energy Cosmic Ray Electrons by the ATIC Balloon Experiment 1.Louisiana State University, Department of.
Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute 84.5% of the total matter in the universe.
