Fig. 3.
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Temporal evolution of various Amaryllis properties: LOIII/LCII (top panel), the ionization parameter Uion (second panel), gas metallicity, Z (third panel), gas number density, n (fourth panel), and star-formation variability, SFR3 Myr/SFR50 Myr (bottom panel). The correlations between LOIII/LCII and each other property are presented in Table 2. The vertical dashed green lines correspond to major merger events, and the dotted red line indicates the snapshot with the highest [OIII]/[CII].
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