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- W2064046248 abstract "Radial velocities of 46 stars in the fields of the globular clusters M 12 (C 1644-018) and M56 (C 1914+300) show that 23 of the stars are cluster members. When these new measurements are combined with all previous ones, the improved cluster velocities are -41.3 ± 1.5 and -134.0 ± 2.7 km s-1, respectively. Six of the observed stars are cluster UV-bright stars. A color-magnitude diagram is constructed for all known UV-bright stars in 29 globular clusters. This composite diagram suggests that UV-bright stars are present in sufficient numbers that they will contribute appreciably to the integrated ultraviolet light of old, metal-poor stellar populations. Although our figure is an improvement over earlier diagrams, it is still seriously incomplete due to selection effects." @default.
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- W2064046248 date "1983-04-01" @default.
- W2064046248 modified "2023-10-18" @default.
- W2064046248 title "Radial velocities of stars in M12 (NGC 6218) and M56 (NGC 6779) and UV-bright stars in globular clusters" @default.
- W2064046248 cites W236706331 @default.
- W2064046248 doi "https://doi.org/10.1086/131153" @default.
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