arXiv · 0708.1716
Age, metallicity and alpha-elements abundance in stellar population
Abstract
We built modelled spectra of stellar population at high resolution and with variable alpha-elements enhancements. Analysing spectra of Galactic globular clusters we show that it is possible to derive reliably and efficiently [Mg/Fe] using spectra integrated along the line-of-sight. These detailed measurements open perspectives for investigating the enrichment process on galaxies and star clusters.
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M. Koleva, R. Gupta, Ph. Prugniel, H. Singh. 2007-08-13. Age, metallicity and alpha-elements abundance in stellar population. https://arxiv.org/abs/0708.1716
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