Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.
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Destruction of the interstellar dust by a supernova
Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.