Models for non-HBL VHE Gamma-Ray Blazars
0. Models for non-HBL VHE Gamma-Ray Blazars. Markus B öttcher Ohio University, Athens, OH, USA. “TeV Particle Astrophysics” SLAC, Menlo Park, CA, July 13 – 17, 2009. Motivation. Until a few years ago, all TeV blazars were high-frequency-peaked BLLac objects (HBLs).
376 views • 23 slides