COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1160 Konkoly Observatory Budapest 1976 July 28 A NEW FLARE STAR IN PISCES While carrying out an objective-prism survey with the Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory, the author discovered a new, large-amplitude flare star. The discovery plate was taken on 1976 June 7. The star abruptly appeared about m_pg = 8.5 at 9:59 UT, and was still well above the plate limit of about m_pg = 10.5 when the exposure ended 14 minutes later. (Accurate timing is possible because the objective- prism spectra are widened with a single trail.) During the flare the object showed a continuous spectrum with the Balmer lines and possibly Ca II K in emission. The star was found at minimum on the Palomar Sky Survey prints at about 15.0 mag, at 1950 position 23h29m09s, -3d01.7'. The figure gives a finding chart for the star, reproduced from the Palomar red print. This new flare star is not only one of the apparently brightest known during outburst, but is also, with a range of more than 6 magnitudes, one of the largest-amplitude flare stars. It deserves further study by optical and radio observers. HOWARD E. BOND * Department of Astronomy University of Washington Seattle, Washington USA and Department of Physics & Astronomy Louisiana State University Baton Rouge, Louisiana USA * Visiting Astronomer, Cerro Tololo Inter-American Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation. [FIGURE 1] Finding chart for the new flare star. The field is a 12' square, reproduced from the Palomar Sky Survey red print. (Copyright by National Geographic Society-Palomar Sky Survey; reproduced by permission.)