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Luminous Blue Variables need not be blue

Published online by Cambridge University Press:  12 April 2016

Cornells de Jager  and
Arnout M. van Genderen
Cornells de Jager
Affiliation:
Laboratory for Space Research Utrecht and Leiden Observatory
Arnout M. van Genderen
Affiliation:
Laboratory for Space Research Utrecht and Leiden Observatory

Abstract

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A number of yellow and red super- and hypergiants show phenomena that are similar to those shown by Luminous Blue Variables. The LBV phenomenon may not be restricted to the blue part of the Hertzsprung-Russell diagram and the conventional name ‘S Dor variables’ seems more appropriate.

Type
Section I: Main Papers, General Discussions, and Two Panel Discussions
Information
International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 127 - 130
Copyright
Copyright © Kluwer 1989

References

Burki, G.: 1978, Astron. Astrophys. 65, 357.Google Scholar
De Jager, C.: 1980. The Brightest Stars, Reidel, Dordrecht.Google Scholar
Fix, J.D., Cobb, M.L.: 1987, Astrophys, J. 312, 290.Google Scholar
Humphreys, R.M., Jones, T.J., Gehrz, R.D. 1987, Astron, J. 94, 315.CrossRefGoogle Scholar
Kholopov, P.N. et al.: 1985, Gen. Cat. of Var. Stars, 4th ed., Nauka, Moscow.Google Scholar
Kukarkin, B.V., et al.: 1974, Gen. Cat. of Var. Stars, 4th ed., Nauka, Moscow.Google Scholar
Maeder, A.: 1980, Highlights of Astron. 5, 473.Google Scholar
Piters, A., De Jager, C., Nieuwenhuijzen, H. 1988, Astron. Aph. 196, 115.Google Scholar
Spaan, F., De Jager, C., Nieuwenhuijzen, H.: 1989, Astron. Aph.; in prep.Google Scholar
Van Genderen, A.M.: 1988, Astron. Astrophys.; in press.Google Scholar