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The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

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Figure

Fig. 1. CO (2-1) profiles of the 2 OH/IR (top, in blue) and 4 carbon stars. The solid line is a fit to the data using Equation 1
Table 1. LMC targets and some properties.
Table 2. Results of the CO J= 2-1 observations.
Table 4. Galactic extreme carbon stars.
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