Photoelectric monitoring of flare stars from 1974 to 1976

Details Photoelectric monitoring of flare stars from 1974 to 1976 Photoelectric monitoring of flare stars from 1974 to 1976

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978tokab.255.2929i&link_type=abstract

Tokyo Astronomical Observatory, Tokyo Astronomical Bulletin, Second Series, no. 255, July 20, 1978, p. 2929-2938.

Astronomy and Astrophysics

Astronomy

Electrophotometry, Flare Stars, Stellar Spectrophotometry, Ubv Spectra, Graphs (Charts), Light Curve, Tables (Data)

Scientific paper

Results are reported for simultaneous UBV photoelectric photometry of the UV Ceti stars AD Leo, EV Lac, UV Cet, WX UMa, V371 Ori, and BD +13 deg 2618. The observations were made in the period from 1974 to 1976. Light curves of some of the observed flares are presented, along with the integrated intensity of each flare and the resulting (U-B) and (B-V) flare colors at maximum light. The observed intensities of UV Cet and EV Lac are corrected for the contributions from the light of their companions.

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