Fine Fluoroscopy on Molecular Clumps Overtaken by Supernova Blast Wave

Physics

Scientific paper

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Chandra Proposal Id #03500728

Scientific paper

By ASCA/BeppoSAX observations of the supernova remnant G78.2+2.1 and IC443, there found three hard X-ray emitting clumps in which efficient electron acceleration would be taking place at the transmitted shock driven by the supernova blast wave. We propose Chandra observations of these newly discovered hard X-ray clumps to uncover the spatial structure of the molecular clumps and to study the particle acceleration in a dense and turbulent medium.

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