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A comparison of the 30 Doradus and η Carinae nebulae

Published online by Cambridge University Press:  14 August 2015

D. J. Faulkner*
Affiliation:
Mount Stromlo Observatory

Extract

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The program of observations of the 30 Doradus and η Carinae nebulae described here had its origin in the general study of Magellanic Cloud nebulae considered in the previous paper. The 30 Doradus nebula is considerably larger and brighter than the other HII regions in the Clouds, and may be treated in greater detail. The η Carinae nebula was chosen as a comparison object in our own Galaxy.

Type
Section II: The Magellanic Clouds
Copyright
Copyright © Australian Academy of Science 1964 

References

Aller, L. H., and Faulkner, D. J. (1962).— P.A.S.P. 74: 219–22.Google Scholar
Aller, L. H., and Liller, W. (1959).— Ap. J. 130: 4556.CrossRefGoogle Scholar
Burgess, A. (1958).— M.N. 118: 477–95.Google Scholar
Liller, W. (1957).— P.A.S.P. 69: 511–17.CrossRefGoogle Scholar
Mathis, J. S. (1962).— Ap. J. 136: 374–80.CrossRefGoogle Scholar
Pottasch, S. R. (1962).— Ap. J. 135: 385–93.CrossRefGoogle Scholar
Seaton, M. J. (1960).— Rep. Progr. Phys. 23: 313–54.CrossRefGoogle Scholar