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Fig. 17
Model water spectra of the 400 GHz lines for W Hya. The layout and scales are as in Fig. 16. The strongest maser activity is found for Ṁ = (1−3) × 10−6 M⊙ yr−1. The mass loss rate derived from the CO lines is 5 × 10−7 M⊙ yr−1.
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