UBV PHOTOELECTRIC PHOTOMETRY FOR FAINT STARS IN THE PLEIADES CLUSTER
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Observatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
Abstract
Photoelectric photometry in the UBV system of Johnson and Morgan was carried out for 30 stars in the Pleiades Cluster. The main sequence between B-V=+0.6 and +0.8 was found to be very narrow, but from then on a broadening of the main sequence is apparent,