Chemodynamical Simulations of Dwarf Galaxy Evolution
Figure 5
Gas density distribution for nine galaxy models differing on the degree of flattening and the initial baryonic mass, after 100 Myr of galactic evolution. The first column represents models with of initial baryonic mass, the middle column shows the gas distribution for models with mass , and the right-hand column displays the models with . The top rows of models are characterised by a roundish initial distribution. The middle rows show models with an intermediate degree of flattening, and the bottom rows are characterised by a flat initial distribution. The left-hand strip shows the (logarithmic) density scale (in g cm−3).
