A computer program for producing synthetic non-LTE molecular spectra from astrochemical models

Joseph Epstein
Context: Molecular transitions can be observed and used to probe the physical and chemical conditions of molecular clouds, which are the building blocks for astrophysical structures. Aims: To provide a tool for analyzing the variation in molecular transition lines throughout a time-dependent chemical model, and for making comparisons between theoretical and observed molecular transitions in non-LTE astrochemical environments. Methods: Data from a time-dependent astrochemical model and its subsequent species abundances, calculated with the NAUTILUS code,...
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