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CNO distributions in the Solar neighborhood with Gaia data

Published online by Cambridge University Press:  07 March 2018

Šarūnas Mikolaitis
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Gražina Tautvaišienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Renata Ženovienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Arnas Drazdauskas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Erika Pakštienė
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Rimvydas Janulis
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Vilius Bagdonas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
Lukas Klebonas
Affiliation:
Institute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257, Vilnius, Lithuania email: Sarunas.Mikolaitis@tfai.vu.lt
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Abstract

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A spread of lifebuilding elements, such as carbon, nitrogen, and oxygen in the Galactic discs is yet not well investigated. In this study, we use spectra from the UVES spectrograph (Gaia-ESO survey ) and the VUES spectograph (SPFOT-PLATO survey) and determine the carbon, nitrogen, and oxygen abundances in FGK stars using the same technique. For some of our target stars the Gaia space observatory has already presented accurate distances, thus we overview the first results of radial and vertical CNO abundance distributions in the Galactic thin and thick disc populations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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