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2006MmSAI..77..864C - Mem. Soc. Astron. Ital., 77, 864-868 (2006)
Are there radical cyanogen abundance differences between galactic globular cluster RGB and AGB stars? Possibly a vital clue to the globular cluster abundance anomaly problem.
CAMPBELL S.W., LATTANZIO J.C. and ELLIOTT L.M.
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Simbad objects: 6
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