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- W1532874037 abstract "Red giant stars are studied on infrared sensitive plates taken with a grism and 4 m CTIO reflector. Each of our regions is 24′ diameter and covers 0.12 sq degrees. We find M5 to M9 stars abundant and carbon and S stars almost non existent in the direction of the galactic center. In two regions (Baade’s window at NGC 6522 and in Sgr I) we have counted more than 1 000 very cool M giants and no C or S stars. Supplementary photography of 10 other regions of the Nuclear Bulge region reveals one genuine C star at 1 = 0° b = −5°6, no S type stars and very large numbers of M stars." @default.
- W1532874037 created "2016-06-24" @default.
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- W1532874037 date "1985-01-01" @default.
- W1532874037 modified "2023-09-27" @default.
- W1532874037 title "Carbon Stars and the Center of our Galaxy" @default.
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- W1532874037 doi "https://doi.org/10.1007/978-94-009-5325-3_20" @default.
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