COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2665 Konkoly Observatory Budapest 13 February 1985 HU ISSN 0374 - 0676 A POSSIBLE NEW FLARE STAR IN THE PLEIADES (M 45) REGION Probably a new flare star in M45 region has been discovered in the course of a photographic survey made with the 16 cm f/5.7 astrograph of the Osservatorio astronomico di Pieve S. Paolo (Lucca) during the autumn 1979. I revealed this object only in October 1983, and a careful plate analysis made by prof. L. Rosino (1984) at Asiago Astrophysical Observatory has proved that the object is very probably a new flare star. The flare star catalogue of Haro et al. (1982) and IBVS from October 1979 onward have been consulted, but the object does not coincide with previous known flare stars. The object lies quite near to TON. new ser. No. 366 = B 539 (about 1'NE). Deep infrared plates taken with the 67/92 cm Asiago Astrophysical Observatory Schmidt camera are empty in the position of this suspected new flare star. Its position has been measured with a micrometer at the Institute di Astronomia dell'universita di Pisa. Its coordinates are: alpha = 3h43.3m; delta = +25d08' +-0.3' (1900) Plate parameters: date - 19 October 1979; T.U. (middle exposure) - 21h48m exposure time - 50 min; emulsion - HP4 (Ilford) The object has a panchromatic magnitude (at max.) = 13. Acknowledgements: Many thanks are due to prof. L. Rosino for the kind interest and helpful suggestions. Thanks are also due to the personnel of the istituto di astronomica dell'universita di Pisa for the use of the micrometer. MATTEO SANTANGELO Monte di Chiatri and Pieve S. Paolo Astrophysical Observatories Casella postale succ. 1, 55100 Lucca - Italy References: Haro, G., Chavira, E., Gonzales, G.: 1982, Bol. obs. Tonantzintla Vol. 3, No. 1, 3 [BIBCODE 1982BITon...3....3H ] Rosino, L.: 1984, Private communication