COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2730 Konkoly Observatory Budapest 24 May 1985 HU ISSN 0374 - 0676 FLARE STARS IN THE PLEIADES According to the programme of regular search for flare stars in the Pleiades region at the National Astronomical Observatory Rozhen of the Bulgarian Academy of Sciences, patrol photographic plates have been taken with the 20"/28" Schmidt telescope in U-light (ZU21 with a UG2 filter) and in pg-light (ZU21 without filter) during the period September 1983 - October 1984. Table I gives some details about the observational material obtained. Table I Telescope Light Time of Number Number of teff. exposure of plates exposures 5 min. 24 140 11h40m U 10 min. 18 101 16h50m 20"/28" pg 5 min. 12 72 6h A new flare star and 6 flare events of known flare stars have been discovered. Table II summarizes our results. The successive columns give the following data: 1. Rozhen designation of the Pleiades flare stars according to Tsvetkov et al. (IBVS, No. 2338, 1983) have been continued; 2. Hertzsprung number; 3.-4. Coordinates for 1900.0; 5.-6. Photographic magnitude at minimum and amplitude of the observed flare events in U-light; 7. Date of the flare event (U.T.); 8. Identification of the flare stars by the Catalog and Identification Charts of the Pleiades Flare Stars (Haro et al., Bol. Inst. Tonantzintla, 3, No. 1, 1982). The identification charts of those new flare stars (R18, R20, R21, R22, R24 - Tsvetkov et al., IBVS, No. 2224, 1982; IBVS, No. 2338, 1983, and the present paper) which are not included in the Tonantzintla Catalog (Haro et al., Table II Rozhen No. HII R.A.1900 D.1900 Umin DeltamU Date Identification R24 3h39.4m 22deg22' 20.2 5.3 30.09.1984 R25 1061 3 40.6 23 48 16.6 2.7 7.09.1984 TC224 R26 1355 3 41.4 23 43 17.3 2.2 7.09.1984 TC262 R9 2411 3 43.7 24 01 16.9 0.7 6.10.1983 TC377 R9 2411 3 43.7 24 01 16.9 2.4 30.09.1984 TC377 R9 2411 3 43.7 24 01 16.9 0.6 1.10.1984 TC377 R27 2602 3 44.3 23 41 18.7 3.2 7.09.1984 TC391 1982) are shown in Figure 1. The scale of the charts corresponds to the scale of the identification charts of Haro et al. (1982). North is at the top, east is to the left. [FIGURE 1] KATYA P. TSVETKOVA, ASSYA G. TSVETKOVA and M.K. TSVETKOV Department of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences, Sofia-1784, Lenin Str. 72 Bulgaria