An empirical spectral library of chemically well characterized stars for stellar population modelling

Bibcode
2012IAUS..284...29D
DOI
10.1017/S1743921312008654
de Castro Milone, André; Sansom, Anne E.; Sánchez-Blázquez, Patricia; Vazdekis, A.; Falcón-Barroso, J.; Allende-Prieto, C.
Bibliographical reference

The Spectral Energy Distribution of Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 284, p. 29-31

Advertised on:
8
2012
Number of authors
6
IAC number of authors
3
Citations
0
Refereed citations
0
Description
With the goal of assembling a new generation of more realistic single stellar population (SSP) models, we have obtained magnesium abundances for nearly 80% of the stars of the widely employed MILES empirical spectral library. Additional spectroscopic observations of carefully selected stars have recently been obtained to improve the parametric coverage of this library. Here we report on: (i) the framework of Mg abundance determination carried out at mid-resolution, (ii) the newly acquired data, and (iii) the preliminary steps towards modelling stellar populations.
Type
Non-refereed
Techniques

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