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- Q6822846 subject Q6441178.
- Q6822846 abstract "The Metallicity distribution function is an important concept in stellar and galactic evolution.It is a curve of what proportion of stars have a particular metallicity ([Fe/H], the relative abundance of iron and hydrogen) of a population of stars such as in a cluster or galaxy.MDFs are used to test different theories of galactic evolution. Much of the iron in a star will have come from earlier type Ia supernovae. Other [alpha] metals can be produced in core collapse supernovae.".
- Q6822846 wikiPageExternalLink McWilliam_contents.html.
- Q6822846 wikiPageWikiLink Q1995140.
- Q6822846 wikiPageWikiLink Q217030.
- Q6822846 wikiPageWikiLink Q3937.
- Q6822846 wikiPageWikiLink Q6441178.
- Q6822846 wikiPageWikiLink Q6472.
- Q6822846 comment "The Metallicity distribution function is an important concept in stellar and galactic evolution.It is a curve of what proportion of stars have a particular metallicity ([Fe/H], the relative abundance of iron and hydrogen) of a population of stars such as in a cluster or galaxy.MDFs are used to test different theories of galactic evolution. Much of the iron in a star will have come from earlier type Ia supernovae. Other [alpha] metals can be produced in core collapse supernovae.".
- Q6822846 label "Metallicity distribution function".