COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2798 Konkoly Observatory Budapest 24 September 1985 HU ISSN 0374 - 0676 TIMES OF MINIMA AND NEW ELEMENTS OF GX LACERTAE GX Lacertae (BD + 56deg2855 = HD 240 055) was discovered as a probable eclipsing binary by Uitterdijk (1934) on photographic plates. Its photometric elements were first determined by Kreiner (1968). No more observations of GX Lac, either photometric or spectroscopic, have been made since 1967. During the period July 1981 - November 1984 GX Lac was observed photoelectrically with the 50 cm reflector at the Cracow Astronomical Observatory. The observations were made using the standard V filter and the star "b" from the Wright's chart of CO Lac (Wright, 1937) was used as a comparison star. From these data three times of minima, as given below, were determined using the tracing-paper method. J.D. hel E O-C1 O-C2 Remarks 2445189.486+/- .003 856 +0.2943 +0.0007 prim. 5993.413+/- 0.05 982.5 +0.3264 -0.0105 sec. 6009.312+/- .003 985 +0.3282 +0.0003 prim. The O-C1 values were calculated using the elements: J.D. 243 9749.3973 + 6.3549d x E (Kreiner, 1968) On the basis of these three minima, the period was corrected P = 6.355243d and the O-C2 values were calculated from the new elements: J.D. 243 9749.3973 + 6.355243d x E For the epoch of the photographic diminishing of brightness of GX Lac, published by Uitterdijk (1934), O-C2=-0.04d, so the period seems to be correct and constant in time. The light curve of GX Lac and orbital elements will be published elsewhere. J.M. KREINER MARIA KRURPINSKA-WINIARSKA Department of Physics M. WINIARSKA Higher pedagogical School Astronomical Observatory Cracow, Poland of the Jagellonian University Cracow, Poland References: Kreiner, J.M., 1968, I.B.V.S. No. 249 Uitterdijk, J., 1934, B.A.N. 7, 160 [BIBCODE 1934BAN.....7..159U ] Wright, F.W., 1937, Harvard Ann., 89, 171 [BIBCODE 1937AnHar..89..171W ]