Volume 622, February 2019
|Number of page(s)||14|
|Published online||28 January 2019|
Systematic investigation of chemical abundances derived using IR spectra obtained with GIANO★
GEPI, Observatoire de Paris, Université PSL, CNRS,
5 Place Jules Janssen,
2 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
3 Crimean Astrophysical Observatory, Nauchny 298409, Crimea
4 Astronomical Observatory, Odessa National University, Shevchenko Park, 65014 Odessa, Ukraine
5 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
6 European Southern Observatory, Casilla 19001, Santiago, Chile
7 Universidad Andrés Bello, Departamento de Ciencias Físicas, Fernandez Concha 700, Las Condes, Santiago, Chile
8 INAF, Osservatorio Astronomico di Bologna, Via Gobetti 93/340129, Bologna, Italy
9 Lund Observatory, Department of Astronomy and Theoretical Physics, Lund University, Box 43, 221 00 Lund, Sweden
10 Zentrum für Astronomie der Universität Heidelberg, Landessternwarte, Königstuhl 12, 69117 Heidelberg, Germany
Accepted: 26 November 2018
Context. Detailed chemical abundances of Galactic stars are needed in order to improve our knowledge of the formation and evolution of our galaxy, the Milky Way.
Aims. We took advantage of the GIANO archive spectra to select a sample of Galactic disc stars in order to derive their chemical inventory and to compare the abundances we derived from these infrared spectra to the chemical pattern derived from optical spectra.
Methods. We analysed high-quality spectra of 40 stars observed with GIANO. We derived the stellar parameters from the photometry and the Gaia data-release 2 (DR2) parallax; the chemical abundances were derived with the code MyGIsFOS. For a subsample of stars we compared the chemical pattern derived from the GIANO spectra with the abundances derived from optical spectra. We derived P abundances for all 40 stars, increasing the number of Galactic stars for which phosphorus abundance is known.
Results. We could derive abundances of 14 elements, 8 of which are also derived from optical spectra. The comparison of the abundances derived from infrared and optical spectra is very good. The chemical pattern of these stars is the one expected for Galactic disc stars and is in agreement with the results from the literature.
Conclusions. GIANO is providing the astronomical community with an extremely useful instrument, able to produce spectra with high resolution and a wide wavelength range in the infrared.
Key words: stars: solar-type / stars: abundances / Galaxy: abundances / Galaxy: disk
© ESO 2019
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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