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The Light Variations of the Red Supergiant Mu Cephei

Published online by Cambridge University Press:  04 August 2017

Luciano Mantegazza*
Affiliation:
Osservatorio Astronomico di Brera Via E. Bianchi 46 22055 Merate Italy

Extract

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The causes of light variations in red supergiants are still discussed. In particular it is not clear if these variations result from deterministic or narrow-band stochastic (pseudo-periodic) processes or from a mixture of both types.

Type
Poster Papers - Sessions 1 and 2
Copyright
Copyright © Reidel 1986 

References

Abramyam, G.V.: 1982, Bull. BYURAKAN Obs. 53, 3;Google Scholar
Coyne, G.V., Kruszewsky, A.: 1968, Astron. J. 73, 20;CrossRefGoogle Scholar
Larsson-Leander, G.: 1962, Arkiv Astron. 3, n.21, 285;Google Scholar
Mantegazza, L.: 1982, Astron. Astrophys. 111, 295;Google Scholar
Polyakova, T.A.: 1975, Variable Stars 20, 75;Google Scholar
Polyakova, T.A.: 1978, Variable Stars 20, 529.Google Scholar