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A new code for comprehensive self-consistent modelling of Planetary Nebula luminescence

Published online by Cambridge University Press:  25 May 2016

V. V. Golovaty ,
Yu.F. Malkov  and
O. V. Rokach
V. V. Golovaty
Affiliation:
1Astronomical Observatory of Lviv State University, Lviv, Ukraine
Yu.F. Malkov
Affiliation:
2Crimean Astrophysical Observatory, Nauchny, Crimea, Ukraine
O. V. Rokach
Affiliation:
1Astronomical Observatory of Lviv State University, Lviv, Ukraine

Extract

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A new code PAN (Photoionized Axially-symmetrical Nebula) for the self-consistent modelling of a cylindrical gaseous nebula photoionized by a central source of ionizing radiation is developed. All of the processes which play an important role in the ionization and thermal equilibrium of the nebular gas are included in the code.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 228
Copyright
Copyright © Kluwer 1997