TiO band strengths in metal-rich globular clusters. VI - NGC 5927 and NGC 6352

Details TiO band strengths in metal-rich globular clusters. VI - NGC 5927 and NGC 6352 TiO band strengths in metal-rich globular clusters. VI - NGC 5927 and NGC 6352

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..800m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Oct. 1984, p. 800-803.

Astronomy and Astrophysics

Astronomy

3

Globular Clusters, Metallicity, Stellar Composition, Stellar Spectra, Giant Stars, Interstellar Extinction, M Stars, Milky Way Galaxy, Stellar Spectrophotometry, Titanium Oxides

Scientific paper

Narrow-band photometry is reported for two clusters of the inner
Galactic halo. The authors obtain [M/H] = -0.4±0.2 for NGC 5927
and [M/H] = -0.5±0.2 for NGC 6352 with E(B-V) = 0m.49
and 0m.29, respectively. These reddening values lead to
consistency with the infrared (giant branch) metallicity scale.

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