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The influence of supernova remnants on the interstellar medium in the large Magellanic cloud seen at 20-600 µm wavelengths
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A stubbornly large mass of cold dust in the ejecta of Supernova 1987A
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, I: dust properties and insights into the origin of the submillimeter excess emission
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, II: gas-to-dust ratio variations across interstellar medium phases
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Surveying the agents of galaxy evolution in the tidally stripped, low metallicity small Magellanic cloud (SAGE-SMC), III: young stellar objects