Mass loss from an extreme OH/IR star: OH 26.5+0.6
Observations of H2O isotopologues of the extreme OH/IR star OH 26.5+0.6 show that the star has an initial mass consistent with it being an intermediate-mass star. The Herschel-HIFI spectra show clear detection of H216O and H217O while H218O is missing, consistent with the prediction of hot bottom burning which occurs in stars with an initial mass
Justtanont, K. et al.
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2017