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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

B. Barbuy ,
A. Milone ,
M. Spite  and
F. Spite
B. Barbuy
Affiliation:
Universidade de Sao Paulo, Depto. Astronomia, CP30627 Sao Paulo, 01051, Brazil
A. Milone
Affiliation:
Universidade de Sao Paulo, Depto. Astronomia, CP30627 Sao Paulo, 01051, Brazil
M. Spite
Affiliation:
Observatoire de Paris, Section d'Astrophysique, 92195 Meudon Pl Cedex, France
F. Spite
Affiliation:
Observatoire de Paris, Section d'Astrophysique, 92195 Meudon Pl Cedex, France

Abstract

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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 

References

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