Chemical content of the circumstellar envelope of the oxygen-rich AGB star R Doradus - Non-LTE abundance analysis of CO, SiO, and HCN

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Fig. 3

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Black: observed main-beam temperature as a function of velocity for 11 rotational transitions of CO (see Table 1). The telescope and rotational quantum numbers are indicated for each line. Red: line profiles resulting from the gas-phase model (see Sect. 4.1.2). The v_LSR of R Dor is 7.5 km s^-1.

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