Fig. 5.
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Left panel: Evolution of mean circularity parameter, ⟨ϵcirc⟩=⟨Jz/Jcirc⟩, with cosmic time (t) and corresponding redshift (z) for Amaryllis. The horizontal dashed line indicates the disk threshold (
, Simons et al. 2019), while the shaded region highlights the triple merger phase. Right panels: Velocity (v) and velocity dispersion (σ) maps of the gaseous disk in [C II] and [O III] emission, showcasing the early gaseous disk properties at z ≃ 11 in FIR emission lines observable with ALMA at these redshifts.
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