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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
Abstract
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
- Copyright
- Copyright © Kluwer 1990