The influence of Population III stars on the early evolution of galaxies |
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Authors: | A A Kabanov B M Shustov |
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Institution: | 1.Institute of Astronomy,Russian Academy of Sciences,Moscow,Russia |
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Abstract: | Numerical simulations of the chemical evolution of disk galaxies taking into account the influence of Population III stars
are considered. The probability that stars with peculiar chemical compositions are present in the solar neigborhood is analyzed,
and possibilities for their detection considered. For various assumptions about the slope of the initial mass function for
Population III stars and the critical metallicity, the radius surrounding the Sun containing at least one such star is 10–12
pc. Such objects could be studied using modern large telescopes. The influence of Population III stars on the chemical evolution
of disk galaxies is investigated. Taking into account the first stars in early stages leads to an earlier onset of chemical
enrichment of the ISM and a characteristic chemical composition of the gas, but all traces of this enrichment have disappeared
by the current epoch. |
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