Circumstellar Nebulae in Young Supernova Remnants


Supernovae descendent from massive stars explode in media that have been modified by their progenitors’ mass loss and UV radiation. The supernova ejecta will first interact with the circumstellar material shed by the progenitors at late evolutionary stages, and then interact with the interstellar material. Circumstellar nebulae in supernova remnants can be… (More)


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@inproceedings{Chu2000CircumstellarNI, title={Circumstellar Nebulae in Young Supernova Remnants}, author={Y Q Chu}, year={2000} }