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Stephen C.-Y. Ng HKU. Outline What are pulsar wind nebulae? Physical properties and evolution Why study PWNe? Common TeV sources, particle accelerators.
Collie Eye Anomaly Progressive Retinal Atrophy Patella Luxation Elbow Dysplasia Heart Valve Disorders Entropion and Ectropion.
Sergio Palomares-Ruiz June 8, 2005 LS N D imits olutions ew iscoveries et’s peak about LSND eutrinos in elphi WIN’05 20th International Workshop on Weak.
Pulsar Wind Nebulae at High Energies
NO º A The NuMI Offaxis º e Appearance Experiment
First Results from MiniBooNE May 29, 2007 William Louis Introduction The Neutrino Beam Events in the MiniBooNE Detector Data Analysis Initial Results Future.
