COMMISSION 27 OF THE I. A. U INFORMATION BULLETIN ON VARIABLE STARS NUMBER 252 Konkoly Observatory Budapest 1968 January 24 NOVA DELPHINI (1967) Since July 12-13, 1967, visual estimates of Nova Delphini have been made by the writers: 1945 estimates on 97 nights by Robinson in Cambridge, Massachusetts, and 522 estimates on 59 nights by Ashbrook in Weston, 10 miles away. The light curve was plotted from the nightly means, provisionally reduced with comparison star magnitudes from the Arizona Tonantzintla Catalogue (Sky and Tele., 30, 1, 24) or the Bright Star Catalogue (3rd edition). Open circles are visual or photovisual observations before the commencement of our series; these were taken from IAUC 2022, 2024, 2025, 2030, and 2036; also, The Astronomer (Ealing, England), 4, 40, 67. [FIGURE 1] Our means agree adequately with photoelectric measures on the same nights by A.J. Stokes and L. Lovell (IBVS 224, 226, and 238), the average deviation being +0.^m048 (comparison with 15 nights of Stokes' observations) and +0.^m065 (15 nights of Lovell's). A similar comparison between Stokes and Lovell gives +0.^m065 (17 nights). These observations are being continued. A definitive reduction of both our series will be submitted to Peremennie Zvezdi. L.J. ROBINSON and J. ASHBROOK "Sky and Telescope" 49 Bay State Rd. Cambridge, Mass. 02138 FLARES OBSERVED AT THE CATANIA ASTROPHYSICAL OBSERVATORY From 22th July 1967 we began photoelectric observations in V light of the flare stare BD +51d2402, EV Lac and PZ Mon collecting, until today, 131 hours of observations. The preliminary results obtained are summarized in the enclosed table. OBSERVED FLARES obs. Date Comp. Star time (JD hel) Delta m rise total Remarke star 2439.. time dur. BD+ BD +51d2402 76.^h4 696.5845 ^m.07 ^d.0035 ^d.0085 unc. 51d2410 EV Lac 39.2 761.4270 .14 double 42d4527 761.4278 .16 .0004 .0038 763.5230 .32 .0004 .0052 854.3048 .92 .0009 .0468 PZ Mon 15.5 754.6521 .11 .0005 .0012 1d1495 Catania, January 24, 1968 S. CRISTALDI, M. RODONO