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</ref><ref name=Casagrande>[http://www.aanda.org/articles/aa/pdf/2011/06/aa16276-10.pdf The Metallicity Distribution Function in the disc of the Milky Way and near the Sun]
</ref><ref name=Frenchaboy>[http://cdsweb.cern.ch/record/529715/files/0112169.pdf The Metallicity Distribution Function of ω Centauri]
</ref><ref name=Halo-Beers-2005>[
</ref><ref name=M31-Sarajedini-2005>[
</ref><ref name=Shlesinger-2011>[
</ref><ref name=Yong2012>{{cite journal|url=
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>{{cite web|url=http://www.astro.bas.bg/~petrov/holzman07_files/ay616/node5.html|title=Chemical evolution models|work=bas.bg|accessdate=3 March 2017}}</ref><ref>{{Cite journal|arxiv=1106.2168|title=<nowiki>The [Fe/H], [C/Fe], and [alpha/Fe] distributions of the Bootes I Dwarf Spheroidal Galaxy</nowiki>|journal=The Astrophysical Journal|volume=738|pages=51|last1= Lai|first1=David K.|author2=Young Sun Lee|last3=Bolte|first3=Michael|last4=Lucatello|first4=Sara|last5= Beers|first5=Timothy C.|last6= Johnson|first6=Jennifer A.|last7=Sivarani|first7=Thirupathi|last8= Rockosi|first8=Constance M.|author-link8=Constance M. Rockosi|year=2011|doi=10.1088/0004-637X/738/1/51|bibcode = 2011ApJ...738...51L }}</ref>
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