Modeling the dust emission from PN IC418
classification
🌌 astro-ph.GA
keywords
dustemissionamountcomparecompositionconstructdepletiondetailed
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We construct a detailed model for the IR dust emission from the PN IC 418. We succeed to reproduce the emission from 2 to 200$\mu$m. We can determine the amount of emitting dust as well as its composition, and compare to the depletion of elements determined for the photoionized region.
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