COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1587 Konkoly Observatory Budapest 1979 April 24 OBSERVATIONS OF V645 CENTAURI AND YZ CANIS MINORIS V 645 Cen The flare star V 645 Cen (R.A.14h26m42s, declination -62d29' (1950), 11.3 visual magnitude at minimum, spectral type dM5e) was observed at Boyden Observatory on the night of 16/17 April 1975. The 41 cm Nishimura reflector was used with an uncooled EMI 6256A photomultiplier tube and a standard Johnson B filter. One low intensity flare was noted during the monitoring period from 19h27m07s U.T. on 16 April to 03h42m15s U.T. on 17 April. (There was an interruption in the observations from 21h54m00s U.T. to 22h01m30s U.T. on 16 April.) YZ CMi The flare star YZ CMi (R.A.07h42m6s, declination +3d41' (1950), 11.6 visual magnitude at minimum, spectral type dM4.5e) was monitored at Boyden Observatory during the night of 22/23 January 1976. Weather conditions were such that worthwile observations were only possible between 19h21m00s and 23h00m00s U.T. One intense flare was recorded during the period. ------------------------------------------------------------------------------------- Flare maximum (I_0+f - I_0)/I_0 = sigma(mag) = (m_lim - m_0) Flare star Universal Time -2.5log|sigma|/I_0 sigma(mag) - 1.19 V 645 Cen 02h53m15s 1.08 2.59 - YZ CMi 20h49m30s 5.14 2.43 1.24 ------------------------------------------------------------------------------------- We are greatly indebted to Prof. F.D.I. Hodgson, the Director of the Institute of Groundwater studies at the university, for access to his department's Hewlett Packard Model 9825 microcomputer and digitizer for the reduction of our data. A.H. JARRETT and J. VAN ROOYEN Boyden Observatory, Astronomy Department University of the Orange Free State Bloemfontein, Republic of South Africa [FIGURE 1]