Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S283(7), p. 452-453, 2011

DOI: 10.1017/s174392131201188x

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Modeling the dust emission from PN IC418

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe 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.

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