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Supergiants in the Magellanic Clouds and in the Galaxy

Published online by Cambridge University Press:  14 August 2015

Th. Walraven  and
J. H. Walraven
Th. Walraven
Affiliation:
Mount Stromlo Observatory
J. H. Walraven
Affiliation:
Mount Stromlo Observatory

Extract

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With the five-colour photometer of the Leiden Southern Station (system V, B, L, U, W) stars can be classified according to luminosity (Th. Walraven and J. H. Walraven 1960).

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 321 - 330
Copyright
Copyright © Australian Academy of Science 1964 

References

Feast, M. W., Thackeray, A. D., and Wesselink, A. J. (1960).— M.N. 121: 337–85.Google Scholar
de Jager, C., and Neven, L. (1957).— Recherches Astron. Obs. Utrecht 13, No. 4.Google Scholar
Johnson, H. L. (1958).— Lowell Obs. Bull. 4: 37–46.Google Scholar
Walraven, Th., and Walraven, J. H. (1960).— B.A.N. 15: 67–83.Google Scholar