COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 2929 Konkoly Observatory Budapest 29 August 1986 HU ISSN 0374 - 0676 NEW FLARE STARS IN ORION We have continued the survey for flare stars in the Orion nebula region. We discovered seven flare stars around the Orion nebula on the plates taken in 1985 with the 40" Schmidt telescope of Byurakan Observatory and from the revision of our old plates. The effective time of observations is about 12 hours (5 hours in B, and 7 hours in U light). ORWO ZU 21 plates with the combination of Schott filters GG385 and UG1 were used. The revisions were carried out on the plates with effective time of observations about 60 hours. Table I gives the data for the seven flare stars found. In the columns of Table I the following data on flares are presented respectively: the Byurakan number of star, coordinates, magnitude at minimum, amplitude, the date of flare, telescope and the identification. The coordinates and magnitudes are approximate. Table I RA (1900.0 ) D (1900.0) M_u deltaM_u Date Telescope B31 5h23m2 -06d58'5 19m3B 5m4B 24.10.85 40" B32 31.0 -06 11.0 20.5 6.0 22.10.85 40" B33 26.1 -04 38.2 (19.0 >4.0 02.12.80 40" B34 31.2 -04 31.8 18.1 2.4 01.12.80 40" B35 22.8 -06 52.1 16.2 2.7 26.02.79 40" B36 26.7 -04 21.1 13.8 1.2 07.03.75 40" N22* B37 34.8 -03 28.6 14.5P9 1.3pg 08.03.75 21" TZ Ori * Andrews, A.D. 1970. Bol. Obs. Tonantzintla-Tacubaya, 34, 195. [BIBCODE 1970BOTT....5..195A ] N.D. MELIKIAN MASSIMO DELLA VALLE Byurakan Observatory Institute of Astronomy, Padova Armenian SSR, University USSR Italy