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

Open Access

Fig. 10

Continuum-subtracted channel maps of W Hya obtained for the ²⁹SiO v = 2 J = 6–5 line at 253.703469 GHz, shown in the same manner as Fig. 3, except that the unit of the color scale is different from other channel maps to show the strong maser emission and weaker emission over the stellar disk.

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