Photoelectric monitoring of flare stars AD Leo, EV Lac and YZ CMi from 1980 to 1984

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photometry, Flare Stars, Ubv Spectra, Brightness, Light Curve, Stellar Flares, Stellar Spectra, Temporal Distribution

Scientific paper

Simultaneous UBV observations of UV Ceti-type flare stars were performed at Tokyo Astronomical Observatory's Okayama Station during 1980-1984. The stars observed were AD Leo, EV Lac, and YZ CMi. A three-color simultaneous photometer with an unrefrigerated EMI 6256 photomultiplier was used. The integrated intensity for each flare computed by integrated U, B, and V light curves in the relative intensity scale is given.

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