Metallicity and gas mass fraction in irregulars and blue compact galaxies - The effect of dark matter

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Compact Galaxies, Dark Matter, Interstellar Matter, Irregular Galaxies, Metallicity, Astronomical Models, Chemical Evolution, Galactic Evolution, Mass To Light Ratios

Scientific paper

We present an attempt to explain the widespread distribution of irregulars and blue compact galaxies in the metallicity (Z) - gas mass fraction (mu) diagram in the framework of the closed-box model of chemical evolution. The differences in Z for the same value of mu among galaxies are ascribable to those in the mass fraction of dark matter which does not participate in the chemical evolution. We evaluate the mass fraction of dark matter for each galaxy required for the simple model to yield the observed metallicity Z for the observed gas mass fraction mu. If a chemical yield of y = 0.01 is adopted, the dark-matter fraction shows good correlations with the mass-luminosity ratio and the dark-matter fraction obtained independently of the chemical evolution. These results lead to the following suggestions: these galaxies contain various fractions of dark matter which do not take part in the chemical evolution; their Z-mu relation follows that of the simple model modified to include the dark matter; and the chemical yield of these galaxies is close to that conventionally used for the chemical evolution of the solar neighborhood.

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