Asteroseismic masses of red giants in M9 and M19 give integrated mass loss values of 0.16 and 0.33 solar masses, with Type II cluster M19 losing more mass than Type I clusters of similar metallicity.
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Asteroseismic Masses of Red Giants in the Galactic Globular Clusters M9 & M19
Asteroseismic masses of red giants in M9 and M19 give integrated mass loss values of 0.16 and 0.33 solar masses, with Type II cluster M19 losing more mass than Type I clusters of similar metallicity.