High-angular-resolution ALMA imaging of the inhomogeneous dynamical atmosphere of the asymptotic giant branch star W Hya - SiO, H2O, SO2, SO, HCN, AlO, AlOH, TiO, TiO2, and OH lines

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Fig. 2

Continuum spectrum of W Hya at 250–268 GHz. The black dots represent the observed continuum fluxes, while the solid red line represents a power-law fit with F_v ∝ v^2.08. The horizontal bars show the bandwidth of the spectral windows, not errors.

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