Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986tokab.276.3187i&link_type=abstract
Tokyo Astronomical Observatory, Tokyo Astronomical Bulletin, Second Series (ISSN 0082-4690), no. 276, July 30, 1986, p. 3187-321
Astronomy and Astrophysics
Astronomy
1
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.
Ichimura Kihachiro
Shimizu Yasuhiro
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