Prefer a chat interface with context about you and your work?
The M dwarf problem: Fe and Ti abundances in a volume-limited sample of M dwarf stars
We report iron and titanium abundance measurements from high resolution spectra in a volume-limited sample of 106 M0 and M0.5 dwarf stars. The sample includes stars north of the celestial equator and closer than 29 parsecs. The results imply that there is an M dwarf problem similar to the previously …