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TiO band strengths in metal-rich globular clusters. VI - NGC 5927 and NGC 6352
1984
Publications of the Astronomical Society of the Pacific
Preserved Fulltext
Narrow-band photometry is reported for two clusters of the inner Galactic halo. We obtain [M/H] = -0.4 ± 0.2 for NGC 5927 and [M/H] = -0.5 ± 0.2 for NGC 6352 with E(B-V) = 0™49 and 0^29, respectively. These reddening values lead to consistency with the infrared (giant branch) metallicity scale.
doi:10.1086/131435
fatcat:rpbpw4v3vbgnjbobbyuqnyypae