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</ref><ref name=Yong2012>[http://arxiv.org/abs/1208.3016 The Most Metal-Poor Stars. III. The Metallicity Distribution Function and CEMP Fraction]</ref>
MDFs are used to test different theories of galactic evolution. Much of the iron in a star will have come from earlier type Ia [[supernova]]e. Other [alpha] metals can be produced in core collapse supernovae.<ref>[http://www.astro.bas.bg/~petrov/holzman07_files/ay616/node5.html Chemical evolution models]</ref><ref>{{
==References==
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