COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1585 Konkoly Observatory Budapest 1979 April 16 SOME INTENSE FLARES OF UV CETI Recent perusal of flare star records at Boyden observatory revealed three intense outbursts from UV Ceti (R.A.=01h36m4, declination = -18d13' (1950), visual magnitude 12,9 at minimum, spectral type dM5,5e) hitherto unreported. The 41 cm Nishimura reflector was used for these observations, fitted with a Johnson B filter. The detector was an uncooled EMI 6256A photomultiplier tube. The flare of (I_0+f - I_0)/I_0 > 8,48 during the observational run on the night of 14 - 15 September was confirmed visually in the 10 cm finder. Reductions from the photometer records were made using a Hewlett Packard Model 9825 microcomputer and digitizer and other computing facilities on the main campus of the Orange Free State university. The flares reported showed the flash phase followed by a more gradual decline characteristic of UV Ceti type flare stars. The following table gives a summary of the observations: -------------------------------------------------------------------------------- 03/04 August 1975: Monitoring Time: 00h40m08s- 03n00m27s U.T. Flare maximum (I_0+f - I_0)/I_0 2.5 log((I_0+f - I_0)/I_0) sigma(mag)=-2.5log|sigma|/I_0 (m_lim - m_0)=sigma(mag)-1.19 U.T. 01h48m15s 2.87 1.15 1.76 0.57 Interruption in observing from:00h07m45s-00h12m45s U.T. 22h58m10s >8.48 >2.32 2.45 1.26 23 11 32 2.19 0.86 2.45 1.26 ------------------------------------------------------------------------------------------------------------------------------------ We wish to express our thanks to Prof. F.D.I. Hodgson, the Director of the Institute of Groundwater Studies at the University, for access to his departments Hewlett Packard microcomputer. A.H. JARRETT and J. van ROOYEN Boyden Observatory Astronomy Department University of The Orange Free State Bloemfontein Rep. of South Africa [FIGURE 1]