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Statistics of flares observed for UV Ceti type stars YZ CMi, AD Leo, and EV Lac at the Okayama Observatory

Published online by Cambridge University Press:  23 September 2016

K. Ishida
K. Ishida*
Affiliation:
Institute of Astronomy, University of Tokyo 2-21-1 Osawa, Mitaka, Tokyo 181 Japan

Abstract

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Photoelectric monitoring of flare stars YZ CMi, AD Leo, and EV Lac has been done at the Okayama Observatory since early 1970s. This is a simultaneous UBV observations with a high time resolution. Some statistics of the flares of the UV Ceti type stars are presented.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 43 - 47
Copyright
Copyright © Kluwer 1990 

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