HII-CHI-mistry is a collection of python subroutines aimed at
the calculation of chemical abundances and physical properties
using emission line fluxes from ionized gaseous nebulae. These
are the available different versions:
. Calculation of oxygen, nitrogen-to-oxygen ratio chemical
abundances and ionization parameter using optical emission
lines both for massive clusters and for Narrow Line Regions of Seyfert 2 galaxies.
. Calculation of oxygen, carbon-to-oxygen chemical
abundances and ionization parameter using ultraviolet
. Calculation of the equivalent effective temperature of the
ionizing source and the ionization parameter using optical
emission lines and the metallicity, if available, as inputs.
Enrique Pérez-Montero. IAA-CSIC
Last update: 2018, December
This program has been made thanks
to the financial support from the Spanish AYA project