In short

An investigation to reconcile star abundances observed in dwarf stars M and FGK-type stars with galactic chemical evolution models.

Trueman, T. C. L. et al. (2026)

Summary

The article addresses discrepancies in chemical abundances derived from low mass stars and proposes ways to reconcile them in the context of the chemical evolution of the Milky Way.

Discussion

Open track for the next club meeting.

See in IOPscience

Automatic translation notice

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