The Gaia-ESO survey: Radial metallicity gradients and age-metallicity relation of stars in the milky way disk
We study the relationship between age, metallicity, and α-enhancement of FGK stars in the Galactic disk. The results are based upon the analysis of high-resolution UVES spectra from the Gaia-ESO large stellar survey. We explore the limitations of the obs
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|Source:||Astronomy and Astrophysics|
|01_Bergemann_The_Gaia-ESO_survey:_Radial_2014.pdf||1.37 MB||Adobe PDF||Request a copy|
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