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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).

Information

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