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Vibrationally excited water emission at 658 GHz from evolved stars

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Academic year: 2021

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Figure

Table 1. Stellar sample and observation dates.
Fig. 1. Spectra of the (0, 1, 0), J = 1 1,0 −1 0,1 transition of water at 658 GHz toward nine Mira-type or semi-regular variables in our sample.
Fig. 3. Spectra of the J = 6−5 transition of 13 CO at 661 GHz toward five stars in our sample, plotted at 1.1 km s −1 resolution (3.0 km s −1 for VY CMa)
Fig. 4. Maser negative optical depths at 22 and 658 GHz in the kinetic temperature and H 2 density plane

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