Authors: A.Bliss, D.M.Worrall, M.Birkinshaw (Bristol), H.Tananbaum, S.Murray (Harvard-Smithsonian C.f.A.) Fig.1: Combined IVU band image, J2310-437 circled.
Radio and X-ray Properties of Magellanic Cloud - Chandra X-Ray ...
Chandra's Clear View of the Structure of Clusters Craig Sarazin University of Virginia Bullet Cluster (Markevitch et al. 2004) Hydra A Cluster (Kirkpatrick.
Igor V. Moskalenko NASA Goddard Space Flight Center [email protected] with Andy W. StrongStepan G. Mashnik Andy W. Strong (MPE, Germany) & Stepan.
Radio galaxies in 6dFGS: influence of the supercluster environment ?
Abell 2256
Extragalactic Science
38 th COSPAR, Bremen – July 18, 2010 :: IVM/Stanford-KIPAC 1 Galactic Cosmic Rays Igor V. Moskalenko Stanford & KIPAC Igor V. Moskalenko Stanford & KIPAC.
Igor V. Moskalenko & Andy W. Strong NASA/GSFC MPE, Germany with Olaf Reimer Bochum, Germany Topics to cover: GALPROP: principles, internal structure, recent.
(2) Profile of the Non-Thermal Filaments of SNRs =>High Energy Particle Acceleration =>High Energy Particle Acceleration In all the SNRs & GC Non Thermal.
Galactic Cosmic Rays
