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CNO distributions in the Solar neighborhood with Gaia data

Published online by Cambridge University Press:  07 March 2018

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

Keywords

Stars:abundancesgalaxy:abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 241 - 242
Copyright
Copyright © International Astronomical Union 2018 

References

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