Chemical and Spectrophotometric Evolutionary Models for Emission Line Star-forming Galaxies
M.L. Mart\'in Manj\'on, M. Moll\'a, A.I. D\'iaz, R. Terlevich
TL;DR
This paper introduces a comprehensive model for star-forming galaxies that integrates chemical evolution, population synthesis, and photoionization to accurately reproduce observed properties of HII galaxies.
Contribution
It presents a novel self-consistent model combining multiple codes to simulate the chemical and spectrophotometric evolution of starbursting HII galaxies.
Findings
Successfully reproduces observed abundances in HII galaxies.
Matches diagnostic diagrams and equivalent width-colour relations.
Provides a unified framework for galaxy evolution modeling.
Abstract
We present a self-consistent model under a star-bursting scenario for H{\sc ii} galaxies, combining different codes of chemical evolution, evolutionary population synthesis and photoionization. The results obtained reproduce simultaneoulsy the observed abundances, diagnostic diagrams and equivalent width-colour relations for local H{\sc ii} galaxies.
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Taxonomy
TopicsSpectroscopy and Laser Applications · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies