CO isotope ratios from ALMA show that six obscured post-AGB stars all have initial masses below 2 solar masses and have undergone very recent, high-rate mass loss.
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ALMA observations of CO isotopologues towards six obscured post-AGB stars
CO isotope ratios from ALMA show that six obscured post-AGB stars all have initial masses below 2 solar masses and have undergone very recent, high-rate mass loss.