COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1926 Konkoly Observatory Budapest 1981 February 18 HU ISSN 0374-0676 FLARE STARS IN ORION Twenty-two new flare stars (Table I) and 8 repeated flares of known flare stars (Table II) had been revealed, while continuing the photographic observations in the Orion nebula region with the Abastumani Observatory 70-cm Meniscus-type telescope, using the multiple exposure method. Table I and II give the data of these flares. We are continuing the numeration of flare stars. Table No alpha1900 delta1900 mpg delta mpg Date 63 5h 30m 28s -4d 09.4' 16.7m 1.0m 27.10.1979 64 31 23 -6 18.6 18.8 2.6 28.10 65 27 45 -6 49.6 16.9 1.1 28.10 66 33 37 -6 16.3 20.4 4.4 28.10 67 26 25 -6 06.5 17.2 1.0 28.10 68 27 08 -4 39.0 21.0 5.4 29.10 69 31 26 -5 45.4 15.2 1.3 16.11 70 23 00 -4 05.6 17.5 9.4 17.11 79 35 02 -6 36.0 16.9 0.7 17.11 72 29 44 -5 47.0 17.6 3.3 17.11 73 23 42 -7 08.5 18.7 1.8 17.11 74 33 53 -4 54.5 17.0 0.6 18.11 75 31 32 -6 08.9 19.4 3.2 25.11 76 28 28 -3 16.5 19.0 3.6 26.11 77 26 57 -5 46.5 17.1 1.2 26.11 78 25 28 -5 03.7 17.7 0.9 27.11 79 30 55 -6 37.2 18.2 3.0 15.12 80 34 46 -3 28.4 15.6 1.6 15.12 81 28 30 -5 58.6 19.1 3.5 15.01.1980 82 29 31 -3 44.8 19.2 3.8 15.01 83 33 08 -7 02.3 19.0 4.3 16.01 84 24 57 -7 03.0 18.5 1.7 16.01 Table II No alpha1900 delta1900 mpg delta mpg Date Ident 1 5h 30m 31s -5d 00.0' 17.0m 1.1m 29.10.1979 Ab 49 2 37 52 -5 52.6 16.3 1.1 17.11 T 254 3 30 44 -7 20.8 15.2 2.5 17.11 T 228 4 30 10 -6 34.1 16.0 1.3 19.11 T 154 5 28 28 -5 36.7 15.5 0.8 25.11 T 194 6 27 32 -4 03.7 17.9 1.8 26.11 T 8 7 27 32 -4 03.7 17.9 1.8 27.11 T 8 8 32 10 -4 50.9 19.1 3.1 16.01.1980 A 47 [FIGURE 1] [FIGURE 2] Out of all registered flares Nos 79, 80, 83 are slow ones, the brightness of which had increased during more than 40 minutes. In Table II the flare stars identified with Tonantzintla (1), Asiago (2) and Abastumani (3) lists are denoted by T, A and Ab, respectively, Outbursts numbered 6 and 7 of the star T8 took place within the time interval 3h 35m. These outbursts are presumably the result of the same flash-activity cycle. Finding charts are given. R. SH. NATSVLISHVILI Abastumani Observatory, Georgia, USSR References: 1. Haro, G. Chavira, E., 1969, Bol. Obs. Tonantzintla y Tacubaya, 5, No. 32, 59 [BIBCODE 1969BOTT....5...59H ] 2. Rosino, L. Pigatto, L., 1969, Contr. Asiago Obs., No. 231 3. Natsvlishvili, R.Sh., Melikian, N.D., 1980, I.B.V.S. No. 1726