Photoionization models of Planetary Nebulae

Abstract

The understanding of astronomical nebulae is based on observational data (images, spectra, 3D data-cubes) and theoretical models. In this review, I present my very biased view on photoionization modeling of planetary nebulae, focusing on 1D multi-component models, on 3D models and on big database of models.

Invited review at the IAU Symposium 323 Planetary Nebulae: Multi-wavelength probes of stellar and galactic evolution

References in corpus (9)

• X-ray enabled MOCASSIN: a 3D code for photoionized media
• A hydrodynamical study of multiple-shell planetary nebulae. III. Expansion properties and internal kinematics: Theory versus observation
• Discovery of Rubidium, Cadmium, and Germanium Emission Lines in the Near-Infrared Spectra of Planetary Nebulae
• Stout: Cloudy's Atomic and Molecular Database
• Deciphering the bipolar planetary nebula Abell 14 with 3D ionization and morphological studies
• The chemical composition of Galactic ring nebulae around massive stars
• Chemical Abundances and Dust in the Halo Planetary Nebula K648 in M15: Its Origin and Evolution based on an Analysis of Multiwavelength Data
• Modelling of aspherical nebulae. I. A quick pseudo-3D photoionization code
• A virtual observatory for photoionized nebulae: the Mexican Million Models database (3MdB)

Cited by in corpus (3)

• The Te[N II]-Te[O III] temperature relation in H II regions and the reliability of strong-line methods
• Exploring the differences of integrated and spatially resolved analysis using integral field unit data: The case of Abell 14
• Morphology and ionization characteristics of planetary nebulae PB 1 and PC 19