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Observational Constraints on Electron Heating at Collisionless Shocks in Supernova Remnants

Observational Constraints on Electron Heating at Collisionless Shocks in Supernova Remnants. Cara Rakowski NRL J. Martin Laming NRL Parviz Ghavamian STScI. H ? emission from the shock front. Non-radiative shocks: primarily H ? emission from the immediate shock front

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Ray precursor - PowerPoint PPT Presentation

Observational Constraints on Electron Heating at Collisionless Shocks in Supernova Remnants