Asymptotic giant branch superwind speed at low metallicity
We present the results of a survey for OH maser emission at 1612 MHz from dust-enshrouded asymptotic giant branch (AGB) stars and supergiants in the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC), with the Parkes radio telescope, aimed
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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