35 AGB stars show iso-dom SiO maser spectra explained by third dredge-up plus low turbulence velocity enabling line-overlap pumping.
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29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
35 AGB stars show iso-dom SiO maser spectra explained by third dredge-up plus low turbulence velocity enabling line-overlap pumping.