Rb-Rich Asymptotic Giant Branch Stars in the Magellanic Clouds
We present high-resolution (R ∼ 60,000) optical spectra of a carefully selected sample of heavily obscured and presumably massive O-rich asymptotic giant branch (AGB) stars in the Magellanic Clouds. We report the discovery of strong Rb I lines at 7800 i
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|Source:||Astrophysical Journal, The|
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