COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1275 Konkoly Observatory Budapest 1977 May 11 CSV 2851 - A RED DWARF VARIABLE CSV 2851 = HV 10814 = BPM 61550 = CoD -38d11343 was introduced in 1973 in the research program on red dwarf variables of the I.T.A. Astronomical Observatory (Ferraz Mello, S. and Torres, C.A.O., 1971 I.B.V.S. 577) after a notes of Sanduleak, N. and Stephenson, C.B. (1973 I.B.V.S. 770) showing that this suspected irregular variable was actually a dM3e star. The star was observed on 9 different nights against the comparison stars CoD -38d11352 and CoD -38d11353. The last one was not very stable, probably due to a nearby faint star that may have been included inadvertently in the diaphragm on some nights. But the observed variation is certainly due to CSV 2851. Although the paucity of the data doesn't permit to obtain unambiguously the period, we represent in Fig. 1 the light curve obtained with the period that best fits the data, P=2.69d. The ordinates are magnitude differences CSV 2851 minus CoD -38d11352 and the individual values are given in Table I. We obtained for the first comparison star a magnitude V=9.40 and a color index B-V=1.23. A B-V=1.54 for CSV 2851 is consistent with a dM3e spectral classification, and if we suppose it to be a normal main sequence star, the visual magnitude of 11.2 would imply a parallax of the order of 0.09". (It is important to confirm this, and we note that the star is less than 1 deg from Gl 646) IVO C. BUSKO GERMANO R. QUAST CARLOS A.O. TORRES Osservatorio Nacional Rio de Janeiro-Brasil [FIGURE 1] Table I JD DeltaB Delta(B-V) 2441000+ 831.670 2.068 0.298 831.677 2.086 0.305 838.635 2.220 0.313 839.617 2.046 0.265 840.621 2.118 0.317 841.695 2.147 0.292 863.612 2.122 0.305 872.586 2.074 0.278 894.489 2.157 0.325 895.507 2.176 0.338