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Publications of the Astronomical Society of Australia
RESEARCH ARTICLE

An Improved Metallicity Calibration with UBV Photometry

S. Karaali A C , S. Bilir B , S. Ak B , E. Yaz B and B. Coşkunoğlu B
+ Author Affiliations
- Author Affiliations

A Beykent University, Faculty of Science and Letters, Department of Mathematics and Computer, Beykent Ayazağa Campus, 34398, Istanbul, Turkey

B Istanbul University, Faculty of Sciences, Department of Astronomy and Space Sciences, 34119, Istanbul, Turkey

C Corresponding author. Email: karsa@istanbul.edu.tr

Publications of the Astronomical Society of Australia 28(2) 95-106 https://doi.org/10.1071/AS10026
Submitted: 14 6 2010  Accepted: 9 2 2011   Published: 16 June 2011

Abstract

We used the data of 701 stars covering the colour index interval 0.32 < B – V ≤ 1.16, with metallicities –1.76 ≤ [Fe/H] ≤ +0.40 dex. The data were taken from the PASTEL catalogue and estimated metallicity-dependent guillotine factors, which provide a more accurate metallicity calibration. We reduced the metallicities of 11 different authors to the metallicities of Valenti & Fischer (2005), and thus obtained a homogeneous set of data which increased the accuracy of the calibration, i.e. [Fe/H] = –14.316δ0.6 2 – 3.557δ0.6 + 0.105. Comparison of the metallicity residuals for two sets of data based on the metallicity-dependent guillotine factors with the ones obtained via metal-free guillotine factors shows that metallicities estimated by means of the new guillotine factors are more accurate than the other ones. This advantage can be used in the metallicity gradient investigation of the Galactic components, i.e. thin disc, thick disc, and halo.

Keywords: stars: abundances, stars: metallicity calibration, stars: metal poor


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