Image Details
Caption: Figure 9.
Comparison of the present-day [M/H] from the AMRs based on the PARSEC and MIST models with the gas-phase oxygen abundances relative to a solar abundance of 12+log(O/H) = 8.69 (M. Asplund et al. 2021). While absolute agreement is not expected between [M/H] in the young stars and the gas-phase oxygen abundance, the enrichment of these different components should be correlated, as confirmed in these data.
© 2026. The Author(s). Published by the American Astronomical Society.