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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

Carney, B.W., Janes, K.A., Flower, P.J. (1985), Astron. J. 90, 1196.Google Scholar
Gustafsson, B., Bell, R.A., Eriksson, K., Nordlund, Å. (1975), Astron. Astrophys. 42, 407.Google Scholar
Richtler, T., Spite, M., Spite, F. (1990), these proceedings.Google Scholar
Russell, S.C., Bessell, M.S. (1989), Astrophys. J. Suppl. 70, 865.Google Scholar
Spite, M., Spite, F. (1990), these proceedings.Google Scholar
Spite, M., Barbuy, B., Spite, F. (1989), Astron. Astrophys. 222, 35.Google Scholar
Spite, M., Cayrel, R., François, P., Richtler, T., Spite, F. (1986), Astron. Astrophys. 168, 197.Google Scholar