Modeling the dust emission from PN IC418

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$\mu$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.

Poster contribution (2 pages, 1 figure) to IAU Symposium 283: "Planetary Nebulae: An Eye to the Future" held in Puerto de la Cruz, Tenerife, Spain in July 25th-29th 2011. Few typos corrected

References in corpus (1)

• Formation of fullerenes in H-containing Planetary Nebulae

Cited by in corpus (2)

• A search for diffuse bands in fullerene planetary nebulae: evidence of diffuse circumstellar bands
• IFU spectroscopy of Southern Planetary Nebulae IV: A Physical Model for IC 418