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Modeling the dust emission from PN IC418
Published online by Cambridge University Press: 30 August 2012
Abstract
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 μm. 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 452 - 453
- Copyright
- Copyright © International Astronomical Union 2012
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