COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 623 Konkoly Observatory Budapest 1972 February 4 A NEW FLARE STAR IN AQUILA In the course of our spectral survey of infrared stars, we notice a 12-magnitude (pg) star, whose spectrum has shown a temporary emission line. The position of the star is (estimated from the positions of BD stars on the PSS) at R.A.=18^h55^m.9; Dec.=+6^06'.5 (1950). Four spectra were obtained on three different nights with the Heidelberg Schmidt Telescope. Kodak 1N plates (behind an RG 5 filter) were used to record the spectral range between 6500A until about 8800A (Ackermann, 1970). On plate no. 436 (see Table), an emission line at, the expected position of H_alpha can be observed. We are tempting to classify the line as H_alpha-line in emission. Plate no. Date Spectrum 435 J.D.2441146.943 M3 439 160.937 Early M, with emission 437 160.967 Early M 466 180.846 M3 Sanduleak (1968) reported that in the spectra of flare stars which he detected spectroscopically, temporary Balmer lines, including H_alpha, in emission can be observed. Unfortunately, we have no spectral plate for the blue spectral regions to check the spectrum of the star in Aquila. However, the appearance of the H_alpha line on plate 436 is accompanied by a decrease in intensity of the spectral regions to the red of that line. Spectral change similar to that observed here, has been detected earlier by Chugainov and Gershberg (Lovell, 1971) in the spectra of genuine flare stars. We want to thank the Director of the Max Planck Institut for Astronomy for the facilities provided to us. B. HIDAJAT M.U. AKYOL Landessternwarte and Max Planck Institut for Astronomy, Heidelberg References: Ackermann, G., Astron. and Astroph., 8, 315, 1970. [BIBCODE 1970A&A.....8..315A ] Lovell, Sir Bernard, Quart. J.R.A.S., 12, 98, 1971. [BIBCODE 1971QJRAS..12...98L ] Sanduleak, N., I.B.V.S. 275, 1968.