The point in the plot showing → alpha element
abundances ([α/Fe]) of a galaxy as a function of the
→ metallicity ([Fe/H]) where the
α-element abundance drops.
The metallicity of the turn-over in α-element abundances
is linked to the → star formation rate
during the early stage of star formation in a galaxy and therefore
also depends on the total mass of the system.
Higher star formation efficiency leads
to higher overall metallicity before the onset of
→ Type Ia supernova → enrichment,
and thus to a knee that is located at higher [Fe/H] values.
See also: → alpha; → element;
→ knee.