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- W3122007067 abstract "We use the self-consistent model technique developed by Martín-Manjón et al. that combines the chemical evolution with stellar population synthesis and photoionization codes, to study the star formation scenarios capable of reproducing the observed properties of star-forming galaxies. The comparison of our model results with a data base of H ii galaxies shows that the observed spectra and colours of the present burst and the older underlying population are reproduced by models in a bursting scenario with star formation efficiency involving close to 20 per cent of the total mass of gas, and interburst times longer than 100 Myr, and more probably around 1 Gyr. Other modes like gasping and continuous star formation are not favoured." @default.
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- W3122007067 date "2011-12-13" @default.
- W3122007067 modified "2023-10-16" @default.
- W3122007067 title "Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios" @default.
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- W3122007067 doi "https://doi.org/10.1111/j.1365-2966.2011.20122.x" @default.
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