Modeling the dust emission from PN IC418

Details Modeling the dust emission from PN IC418 Modeling the dust emission from PN IC418

2011-10-11

arxiv.org/abs/1110.2328v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

Poster contribution (2 pages, 1 figure) to IAU Symposium 283: "Planetary Nebulae: An Eye to the Future" held in Puerto de la C

Scientific paper

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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