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Stellar Feedback, AGN Feedback and Fluid Microphysics in Galaxy Evolution

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Figure

Figure 2.3: Density distributions of outflows and gas in different phases as in Fig. 2.2,but for m10v and m09
Figure 3.1: Star formation rates(SFRs) as a function of time in
Figure 3.2:Total stellar mass as a function of time in each of our simulations(each IC from Table 3.1, as labeled)
Figure 3.5: Images of the gas morphology of the cosmological simulations at zasa slightly higher accretion rate in the outer disc of this simulated galaxy
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