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Carbon and nitrogen in the cool supergiant A7 of the young globular cluster NGC 330 in the SMC
Published online by Cambridge University Press: 19 July 2016
Abstract
C2 and CN bands in the wavelength region λ 560 - 680 nm were used to obtain the carbon and nitrogen abundances in the supergiant star A7 of the young, metal-poor, globular cluster NGC 330 in the Small Magellanic Cloud (SMC).
- Type
- Stellar Evolution
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 370 - 371
- Copyright
- Copyright © Kluwer 1991