Circumstellar Nebulae in Young Supernova Remnants

Abstract

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)

Topics

3 Figures and Tables

Cite this paper

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