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Stella Offner edited Conclusion [1].tex
almost 10 years ago
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\section{Conclusion} \section{Conclusions}
We have shown that the mass of a stellar outflow cannot be inferred from observations in ^{12}CO but that the velocity and structure can. To determine the mass, observations in the optically thin ^{13}CO are needed, and these observations will also significantly improve the data on the velocity and structure of the outflow.