Abstract
We have obtained additional and improved UBVRI photometric data for BS 655 and BS 6555. The program has consisted of 171 observations of standard stars, 370 of comparison stars and 218 of each component of p Draconis. The results indicate a high quality set of photometric measurements which show that during the observations neither BS 655 nor BS 6555 suffered light variations larger than 0.005 mag. Key words: METALLIC-LINE STARS - VARIABLE STARS - PHOTOMETRY.
