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<p>are observable around the Milky Way. As a result of the buildup from an assortment of satellite galaxies, variations in properties such as <a href="page.php?w=metallicity">metallicity</a> are present across stellar populations in halos.</p>

<p><a href="page.php?w=Astrophysical_simulations">Astrophysical simulations</a> of galaxies have predicted that stellar halos should have two components: an inner region dominated by stars which formed within the galaxy, and an outer region primarily composed of stars accreted through merger events. Predictions</p><p>
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