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On Variations in the Flare Activity of V 1054 Oph

Published online by Cambridge University Press:  14 August 2015

W. E. Kunkel
W. E. Kunkel*
Affiliation:
Cerro Tololo Inter-American Observatory∗, La Serena, Chile

Extract

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Four years ago I examined the flare incidence data then available for UV Ceti and V1054 OPH (Wolf 630) and concluded that no evidence could be found for periodic or secular variation in the levels of activity (Kunkel, 1971). Variations greater than 0.3 mag. (rms) should have been found.

Type
Part 1 / Flare Stars and T Tauri Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 67 - 68
Copyright
Copyright © Reidel 1975 

References

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Kunkel, W. E.: 1971, Bull. Am. Astron. Soc. 3, 13.Google Scholar
Kunkel, W. E.: 1973, Astrophys. J. Suppl. 25, 1.Google Scholar
Kunkel, W. E.: 1975, this volume, p. 15.Google Scholar