The Ca II triplet in red giant spectra: [Fe/H] determinations and the role of [Ca/Fe]

Date

2016

Authors

Da Costa, Gary

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Publisher

Blackwell Publishing Ltd

Abstract

Measurements are presented and analysed of the strength of the Ca II triplet lines in red giants in Galactic globular and open clusters, and in a sample of red giants in the LMC disc that have significantly different [Ca/Fe] abundance ratios to the Galactic objects. The Galactic objects are used to generate a calibration between Ca II triplet line strength and [Fe/H], which is then used to estimate [Fe/H]CaT for the LMC stars. The values are then compared with the [Fe/H]spec determinations from high-dispersion spectroscopy. After allowance for a small systematic offset, the two abundance determinations are in excellent agreement. Further, as found in earlier studies, the difference is only a very weak function of the [Ca/Fe] ratio. For example, changing [Ca/Fe] from +0.3 to −0.2 causes the Ca II-based abundance to underestimate [Fe/H]spec by only ∼0.15 dex, assuming a Galactic calibration. Consequently, the Ca II triplet approach to metallicity determinations can be used without significant bias to study stellar systems that have substantially different chemical evolution histories.

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Source

Monthly Notices of the Royal Astronomical Society

Type

Journal article

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Access Statement

Open Access

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