The Interaction of Supernova Remnant in the Early Phase with a Circumstellar Shell
The observations in the ultraviolet(IUE), the near infrared(speckle interferometry), and the soft X-ray(Ginga) of SN1987A suggest circumstellar shells(CSSs) exist. The shells have been formed when the fast blue supergiant wind sweeps the red supergiant wind.
KeywordsRarefaction Wave Supernova Remnant Speckle Interferometry Azimuthal Wave Numerical Result Figure
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