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- W2013499347 abstract "We present a simple empirical model which reproduces the observed mid-1R continuum emission of the planetary nebula NGC 7027. The model includes free-free emission and continuum emission from cold and warm amorphous carbon grains. We have used the laboratory measured properties of amorphous carbon grains. The spectrum is modeled between 2 μm and 1 mm and provides evidence that hot amorphous carbon grains provide the bulk of the mid-I R continuum emission." @default.
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- W2013499347 title "Mid-IR continuum in NGC 7027: evidence for the presence of hot amorphous carbon grains" @default.
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- W2013499347 doi "https://doi.org/10.1016/0032-0633(95)00026-2" @default.
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