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We describe the propagation of supernova shocks within the surroundingmedium, which may be due to mass-loss from the progenitor star. The structureand density profile of the ejected material and surrounding medium areconsidered. Shock wave interaction with clouds and wind-bubbles, and issuesrelevant to cosmic rays are briefly discussed.

Supernova Propagation in the Circumstellar and Interstellar Medium