UBV photometry of flare stars in the Pleiades

Details UBV photometry of flare stars in the Pleiades UBV photometry of flare stars in the Pleiades

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975afz....11..565c&link_type=abstract

Astrofizika, vol. 11, Nov. 1975, p. 565-578. In Russian.

Astronomy and Astrophysics

Astronomy

9

Constellations, Pleiades Cluster, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Astronomical Catalogs, Background Radiation, Main Sequence Stars, Photographic Plates, Schmidt Telescopes, Stellar Luminosity

Scientific paper

Results are presented for UBV photometry of 283 flare stars at minimum light in the Pleiades region. A technique is developed and used to take account of background effects during photographic UBV photometry with an iris microphotometer. The data obtained show that the Pleiades flare stars are located on both sides of the main sequence on the (V, B-V) color-luminosity diagram, but are mostly located above the main sequence on the (U-B, B-V) diagram. It is noted that this distribution is almost the same as that for flare stars in the Orion association.

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