Modelling of aspherical nebulae. I. A quick pseudo-3D photoionization code
arXiv:astro-ph/0503082 · doi:10.1111/j.1365-2966.2005.09049.x
Abstract
We describe a pseudo-3D photoionization code, NEBU_3D and its associated visualization tool, VIS_NEB3D, which are able to easily and rapidly treat a wide variety of nebular geometries, by combining models obtained with a 1D photoionization code. The only requirement for the code to work is that the ionization source is uniqu e and not extended. It is applicable as long as the diffuse ionizing radiation f ield is not dominant and strongly inhomogeneous. As examples of the capabilities of these new tools, we consider two very differ ent theoretical cases. One is that of a high excitation planetary nebula that ha s an ellipsoidal shape with two polar density knots. The other one is that of a blister HII region, for which we have also constructed a spherical model (the sp herical impostor) which has exactly the same Hbeta surface brightness distrib ution as the blister model and the same ionizing star. These two examples warn against preconceived ideas when interpreting spectroscop ic and imaging data of HII regions and planetary nebulae. The tools NEBU_3D and VIS_NEB3D, which will be made publicly available in the future, should facilitat e the performance of numerical experiments, to yield a better understanding of t he physics of aspherical ionized nebulae.
11 pages, 19 figures (mainly in color). Accepted by MNRAS
References in corpus (14)
- Mocassin: A fully three-dimensional Monte Carlo photoionization code
- A 3D Monte Carlo Photoionization Code for Modeling Diffuse Ionized Gas
- Nebular Abundance Errors
- Observations and 3D photoionisation modelling of the Wolf-Rayet planetary nebula NGC 1501
- Three-dimensional photoionization modelling of the planetary nebula NGC 3918
- Three-dimensional photoionisation modelling of the hydrogen-deficient knots in the planetary nebula Abell 30
- A photoionization model of the compact HII region G29.96-0.02
- The physical parameters, excitation and chemistry of the rim, jets and knots of the planetary nebula NGC 7009
- Morphology and kinematics of Planetary Nebulae II. A Diabolo model for NGC 3132
- Molecular Counterparts of Ultracompact HII Regions with Extended Envelopes
- 3-D Photoionization Structure and Distances of Planetary Nebulae IV. NGC 40
- 3-D Photoionization Structure and Distances of Planetary Nebulae I. NGC6369
- The Structure and Star-Formation History of NGC 5461
- 3-D Photoionization Structure and Distances of Planetary Nebulae II. Menzel 1
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- Photoionization models of Planetary Nebulae
- Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning
- An atlas of synthetic line profiles of planetary nebulae