The Mid-IR Emission Structure of IRAS 16594-4656
Abstract
We report TIMMI2 diffraction-limited mid-IR images of the multipolar PPN IRAS 16594-4656. By using the Lucy-Richardson deconvolution algorithm we recover a two-peaked morphology in the innermost region at 8.6 and 11.5 microns. We interpret the observed mid-IR structure as the detection of the two limb-brightened peaks indicating the presence of a dusty toroidal structure in IRAS 16594-4656. We find that the supposed biconical openings of the dust torus are in good agreement with one of the bipolar outflows identified in the HST optical images.
Keywords
Cite
@article{arxiv.astro-ph/0402064,
title = {The Mid-IR Emission Structure of IRAS 16594-4656},
author = {D. A. Garcia-Hernandez and A. Manchado and P. Garcia-Lario and Antonio Benitez Canete and J. A. Acosta-Pulido and A. M. Perez Garcia},
journal= {arXiv preprint arXiv:astro-ph/0402064},
year = {2007}
}
Comments
4 pages, 2 figures, to appear in the conference proceedings of the Asymmetric Planetary Nebulae III. Winds, Structure, & the Thunderbird (Eds. M. Meixner, J. Kastner, N.Soker and B. Balick) held 28 July - 2 August, 2003. ASP Conference Series (in press)