COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2209 Konkoly Observatory Budapest 1982 October 18 HU ISSN 0374-0676 PHOTOELECTRIC OBSERVATIONS OF THE FLARE STAR BY Dra IN 1977 Continuous photoelectric monitoring of the flare star BY Dra has been carried out at the Stephanion Observatory (l=-22deg49'44",phi=+37deg45'15") during the year 1977, using the 30-inch Cassegrain reflector of the Department of Geodetic Astronomy, University of Thessaloniki. Observations have been made with a Johnson dual channel photoelectric photometer in the B colour of the international UBV system. The telescope, the photometer and the observational procedure have been described elsewhere (Mavridis et al., 1981). Here we mention only that the transformation of our instrumental ubv system to the international UBV system is given by the following equations: U = v0 -0.016(b-v)0 + 1.227, B-U = 0.684 + 1.057(b-v)o , U-B =-1.521 + 0.979(u-b)0 . The monitoring intervals in UT as well as the total monitoring time for each night are given in the Table I. Any interruption of more than one minute has been noted. Table I Monitoring intervals in 1977 Date Monitoring Intervals (U.T.) Total Monitoring Time 1977 July 7 20h15m - 20h45m,20h47m - 21h25m, 21h27m - 22h27m. 02h 08m 8 19 29 - 20 04, 20 07 - 20 36 , 20 38 - 21 07, 21 57 - 22 23. 01 59 10 20 40 - 21 18, 21 20 - 21 53, 21 55 - 22 22. 01 38 Total 1977 05h 45m =05.75h During the 5.75 hours of the monitoring time no flare was observed. Acknowledgements: The support of the National Hellenic Research Foundation for this research is gratefully acknowledged. L.N. MAVRIDIS and P. VARVOGLIS Department of Geodetic Astronomy University of Thessaloniki Reference: Mavridis, L.N., Asteriadis, G., and Mahmoud, F.M.: 1982, in E. Mariolopoulos, P.S. Theocaris, and L.N. Mavridis (Editors) Compendium in Astronomy, D. Reidel, Dordrecht-Holland, p. 253. [BIBCODE 1982coas.conf..253M ]