Mg/Fe ratio of MILES stars (Milone+, 2011)

Details Mg/Fe ratio of MILES stars (Milone+, 2011) Mg/Fe ratio of MILES stars (Milone+, 2011)

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..74141227m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/414/1227. Originally published in: 2011MNRAS.414.1227M

Computer Science

Stars: Nearby, Abundances

Scientific paper

We have obtained [Mg/Fe] measurements for 76.3 per cent of the stars in the Mid-resolution Isaac Newton Telescope Library of Empirical Spectra (MILES) spectral library used for understanding stellar atmospheres and stellar populations in galaxies and star clusters. These abundance ratios were obtained through (1) a compilation of values from the literature using abundances from high-resolution (HR) spectroscopic studies and (2) a robust spectroscopic analysis using the MILES mid-resolution (MR) optical spectra. All the [Mg/Fe] values were carefully calibrated to a single uniform scale, by using an extensive control sample with results from HR spectra.
(2 data files).

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