We present a new calibration of the CaII triplet as metallicity indicator based in 4 globular and 11 open clusters which cover a range of metallicity - 2≤[Fe/H]≤+0.1 and age 13≤(Age/Gyr)≤0.25. We use it to derive the metallicity distribution in two fields situated at 5 and 8 degrees from the center of the LMC. We show that the mean [Fe/H] of the LMC field decreases as we move away from the bar. © 2006 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Carrera, R., Gallart, C., Pancino, E., Zinn, R., & Hardy, E. (2006). The metallicity distribution and its gradients in the LMC via calcium triplet spectroscopy. ESO Astrophysics Symposia, 2006, 230–231. https://doi.org/10.1007/978-3-540-34136-9_77
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