We construct a detailed model for the IR dust emission from the PN IC 418. We succeed to reproduce the emission from 2 to 200μm. 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.
Cite
@article{arxiv.1110.2328,
title = {Modeling the dust emission from PN IC418},
author = {Christophe Morisset and Ryszard Szczerba and D. A. Garcia-Hernandez and Pedro Garcia-Lario},
journal= {arXiv preprint arXiv:1110.2328},
year = {2015}
}
Comments
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