Fig. 8
Important molecular contributions in the spectrum of an M-type AGB star, in the wavelength region 0.3–1.35 μm (left panel) and 1.0–3.9 μm (right panel), calculated for a hydrostatic model atmosphere with L = 5000 L⊙, T⋆ = 2800 K, M = 1 M⊙. The different photometric bands are also marked.
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