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Spectroscopic work in the Magellanic Clouds: NGC 330 in the SMC

Published online by Cambridge University Press:  14 August 2015

M. W. Feast
M. W. Feast*
Affiliation:
Radcliffe Observatory

Extract

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This paper gives the results of a spectroscopic study of individual stars in the SMC cluster NGC 330. Before this, however, it may be useful to review briefly the spectroscopic evidence bearing on the questions of reddening and chemical composition in the Magellanic Clouds—matters about which there has not been entire agreement in the past.

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 330 - 334
Copyright
Copyright © Australian Academy of Science 1964 

References

Arp, H. C. (1958).— A.J. 63: 273–82 and 487–91.Google Scholar
Arp, H. C. (1959).— A.J. 64: 175–82 and 254–8.Google Scholar
Buscombe, W., and Kennedy, P. M. (1962).— J.R.A.S. Canada 56: 113–23.Google Scholar
Feast, M. W. (1960).— Observatory 80: 104–6.Google Scholar
Feast, M. W. (1961).— Observatory 81: 73–4.Google Scholar
Feast, M. W., Thackeray, A. D., and Wesselink, A. J. (1960).— M.N. 121: 337–85.Google Scholar
Feinstein, A. (1959).— Zs.f. Ap. 47: 218–24.Google Scholar
Johnson, H. L. (1958).— Lowell Obs. Bull. 4: 37–46.Google Scholar
Wesselink, A. J. (1961).— M.N. 122: 503–7.Google Scholar
Wesselink, A. J. (1962).— M.N. 124: 359–69.Google Scholar