Fig. 1

Cross-sectional snapshots of a DARWIN model for a C-type AGB star, with M* = 1 M⊙, log L* ∕L⊙ = 4.00, T* = 2600 K, up = 6 km s−1, and [Fe∕H] = −1.0 (SMC). Upper, middle, and lower panels: gas density, dust density, and velocity of the gas (negative velocity inward), respectively. The panels show atmospheric snapshots at maximum (left column, ϕ = 0.0) and minimum (right column, ϕ = 0.5) luminosity. The solid black line indicates the radius of the star, calculated from the Stefan–Boltzmann law.
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