The 2.5-Dimensional Photoionization Code ``PAN'' for Modeling of Axially Symmetric Nebulae: The Distinctive Features

Details The 2.5-Dimensional Photoionization Code ``PAN'' for Modeling of Axially Symmetric Nebulae: The Distinctive Features The 2.5-Dimensional Photoionization Code ``PAN'' for Modeling of Axially Symmetric Nebulae: The Distinctive Features

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..804...66r&link_type=abstract

PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP Conference Pr

Astronomy and Astrophysics

Astronomy

Planetary Nebulae, Stellar Composition, Photoionisation, Astronomy Computing, Computer Aided Analysis, Planetary Nebulae, Abundances, Chemical Composition, Atomic Processes And Interactions, Molecular And Chemical Processes And Interactions, Mathematical Procedures And Computer Techniques

Scientific paper

A multi-purpose spectrum synthesis code ``PAN'' (``Photoionized
Axisymmetric Nebula'') is presented. The code allows computing of
self-consistent steady-state models of morphologically-realistic
axisymmetric gaseous, dust or gas+dust envelopes. Only the main features
of the code ``PAN'' are enumerated here.

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