COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1266 Konkoly Observatory Budapest 1977 April 18 FLARE ACTIVITY ON G12-30 We have observed two prominent flares on the star G12-30 (RA= 12h16m31s Dec.= 11d24.0',1950) during seven nights of monitoring it as part of a survey of nearby late M dwarfs. Photometric observations were made in the B-band of the UBV system using the 60-inch (1.5 m) telescope of the Hale Observatories at Mt. Wilson. Time resolution was limited to ten-second integrations. The sky background was measured at three minute intervals. After subtracting the sky background, the signal was ratioed to the quiescent state of the object. A total time of 14.6 hours was spent integrating on the object itself during the periods February 9-11 and February 26 - March 1, 1977 (UT). Harrington et al. (1975) list the following data for G12-30: m_v = 13.79 B-V = 1.83 pi = 0.151" which implies that the object is a late M dwarf. Image tube spectra previously obtained by Veeder (unpublished) indicate a late M type with strong H-alpha in emission. Thus, G12-30 is probably a UV Ceti type flare star. This paper presents the results of one phase of research carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract NAS 7-100, sponsored by the National Aeronautics and Space Administration. [FIGURE 1] [FIGURE 2] GLENN J. VEEDER * OLAV L. HANSEN ** * Guest Investigator,Hale Observatories California Institute of Technology and Carnegie Institution of Washington ** National Research Council, Resident Research Associate References: Harrington, R.S., Dahn, C.C., Behall, A.L., Priser, J.B., Christy, J.W., Riepe, B.Y., Ables, H.D., Guetter, H.H., Hewitt, A.V. and Walker, R.L. (1975), Publ. U.S. Naval Observatory, Vol. XXIV, Part 1 [BIBCODE 1975PUSNO..24a...1H ]