Image Details
Caption: Figure 19.
Comparison between MWM DR19 and APOGEE DR17 abundances as a function of Teff color coded by MWM [M/H]. S/N was restricted to be larger than 50 in both surveys. Abundances of Cglobal and Nglobal are from the global fit. The solid black line shows the running median value.
© 2025. The Author(s). Published by the American Astronomical Society.