Molecules, shocks, and disk in the axi-symmetric wind of the MS-type AGB star RS Cancri

Open Access

Fig. 19

Population diagram for SO₂. The three data points in brackets correspond to the three lowest frequency SO₂ lines observed with setup 1, which, due to a different uv coverage, resulted in a comparably larger beam than the setup 2 observations (see Table 2 and Eq. (6)).

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