Chemodynamical Simulations of Dwarf Galaxy Evolution

<table>The metallicity of a galaxy, as a function of time, for models with metal-enriched galactic winds. This plot shows the solution of (<a href="https://static.hindawi.com/articles/aa/volume-2014/750754/figures/#EEq16">16</a>) for three different values for the enrichment parameter <svg height="7.9499998" id="M228" style="vertical-align:-0.1638pt" version="1.1" viewbox="0 0 9.7749996 7.9499998" width="9.7749996" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
<g transform="matrix(.017,-0,0,-.017,.062,7.675)"><path d="M545 106q-67 -118 -134 -118q-24 0 -40 37.5t-30 129.5h-2q-47 -72 -103 -119.5t-108 -47.5q-47 0 -76 45.5t-29 119.5q0 113 85 204t174 91q47 0 70 -33.5t43 -119.5h3q32 47 80 140l55 13l10 -9q-47 -80 -138 -201q17 -99 27.5 -136t22.5 -37q23 0 69 61zM333 204
q-14 98 -31 149.5t-50 51.5q-49 0 -94 -70t-45 -164q0 -55 15.5 -86t40.5 -31q70 0 164 150z" id="x1D6FC"></path></g>
</svg>.</table>

Advances in Astronomy

Chemodynamical Simulations of Dwarf Galaxy Evolution

Figure 6