COMMISSION 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 3836 Konkoly Observatory Budapest 4 February 1993 HU ISSN 0374 - 0676 A FLARE EVENT ON THE A-TYPE STAR BD+47d819 A flare phenomenon was detected on the 60/90cm Schmidt telescope of Beijing Astronomical Observatory on January 9, 1992. Kodak 103aO plates and UG2 filter were used during the observation. Each plate included 6 exposures of each object. The exposure time for every single point was 10 minutes. By using the CCD plate-measuring instrument, set up in the laboratory, of the infrared astronomical group of BAO, I discovered a flare event and identified the star with BD+47d819. It is near the open cluster a Persei. Figure 1 presents the finding chart of the star. The V magnitude of the star was 9.25, and B-V=0.413 (Prosser, 1992). Its spectral type was A7 in CSI Catalog, and A5 in Fehrenbach's list (1987). The normal U magnitude on the plates was about 10.0 mag., and the flare one was around 8.5 mag. Figure 2 shows the photographic reproduction of the flare event of BD+47d819. The maximum brightness appeared in the interval between 11h41m00s and 11h51m00s (U.T.). [FIGURE 1] Figure 1. Finding chart of BD+47d819 [FIGURE 2] Figure 2. Photographic reproduction of the flare event of BD+47d819 I shall make further observations so as to understand the characteristics of the star better. Jun-jie WANG Beijing Astronomical Observatory, Chinese Academy of Sciences Beijing 100080 China References: Catalog of Stellar Identifications, CDS, Strasbourg, 1979 Fehrenbach, Ch. et al., 1987, A. A. Suppl. Ser., 68, 515. [BIBCODE 1987A&AS...68..515F ] Prosser, C. F., 1992, Astron. J., 103, 488. [BIBCODE 1992AJ....103..488P ]