Abstract
We present abundance studies of dwarf irregular galaxies in the Local Group which appear to have undergone very slow chemical evolution since they have low nebular abundances, but have had ongoing star formation over the past 15 Gyr. They are too distant for red giant abundance analyses to examine the details of their chemical evolution. However the isolated, bright blue supergiants do allow us to determine their present-day iron abundances. We compare the [α/Fe] ratios in the dwarf irregulars to those from recent analyses of red giant branch stars in dwarf spheroidal galaxies, damped Lyman α absorption systems, and the latest model predictions.
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Kaufer, A., Venn, K., Tolstoy, E., Kudritzki, R. (2006). Abundances in Local Group Early-Type Stars. In: Randich, S., Pasquini, L. (eds) Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-34136-9_74
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DOI: https://doi.org/10.1007/978-3-540-34136-9_74
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