Fig. 3
Download original image
Exemplary elemental abundances of the selected sample of M dwarfs (up to 43 in total) in the [X/H]–[Fe/H] space, compiled from the APOGEE (Souto et al. 2017, 2018, 2022), Subaru/IRD (Ishikawa et al. 2022), and CARMENES (Ishikawa et al. 2020) surveys. The numbers of M dwarfs from these individual surveys are shown for individual elemental pairs. See Fig. B.2 for the full set of selected M-dwarf abundance data.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.