``DIOGEN'' - A New Computing Tool for the Diagnostics and Chemical Analysis of Nebular Plasma

Astronomy and Astrophysics – Astronomy

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Planetary Nebulae, H Ii Regions, Plasma Diagnostics, Astronomy Computing, Computer Aided Analysis, Stellar Composition, Element Relative Abundance, Planetary Nebulae, Hii Regions, Emission And Reflection Nebulae, Mathematical Procedures And Computer Techniques, Magnetohydrodynamics And Plasmas, Abundances, Chemical Composition

Scientific paper

A new software tool ``DIOGEN'' (DIagnostics Of GasEous Nebulae) has been developed to derive the physical conditions (Ne, Te and ionic abundances) as well as the chemical abundances in a low-density (nebular) plasma. The plasma diagnostics are based on a wide set of ions and emission lines and utilize several new techniques as well as classical ones. The code ``DIOGEN'' is running under both MS Windows and Linux and may be used for nebular diagnostics and abundance determinations in planetary nebulae and HII regions.

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