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- W3004432006 abstract "Integrated CCD spectra in the 3850-4200 A region were obtained for nine metal-rich globular clusters in M31. The spectra are analyzed using the reddening-free spectral-classification system of Rose (1984). The data are combined with data obtained by Rose and Tripicco (1986) for nine metal-rich Galactic globular clusters and with spectra of 72 stars with well-determined atmospheric parameters. It is found that the 4000 A light from metal rich M31 globulars is dominated by dwarfs, while giants and dwarfs contribute equally to the light from the mean of the metal-rich Galactic globulars. The contribution of early-type stars to the 400 A light from M31 clusters is less than 5 percent in most cases. Also, the 3883 and 4216 CN bands in the M31 globulars are very strong for their integrated spectral types. The results suggest that the metal-rich M31 globular clusters are much younger than Galactic metal-rich clusters like 47 Tuc or M71. 75 references." @default.
- W3004432006 created "2020-02-14" @default.
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- W3004432006 date "1986-09-01" @default.
- W3004432006 modified "2023-10-18" @default.
- W3004432006 title "Spectroscopy of Metal-Rich M31 Globular Clusters" @default.
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