COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 185 Konkoly Observatory Budapest 20 February 1967 NEW VARIABLE STARS During a survey of variable stars, on plates taken with the Schmidt telescope 40/50/100 of Asiago Astrophysical Observatory. I have found the following new variable stars: var RA 1900 D Max min type GR 120 11h32m07s +56d50' 16.7 17.4 RR GR 121 11h34m15s +54d37' 16.5 17.5 RR GR 122 11h34m22s +55d42' 16.7 17.5 RR GR 123 11h52m47s +55d48' 15.7 17.0 RR GR 122 is near to a small galaxy. Padua Observatory, Italy G. ROMANO PHOTOELECTRIC OBSERVATIONS OF TX UMa Three photoelectric minima of TX UMa, obtained at the Nurnberg Observatory in the years 1965, 1966 and 1967 show large negative O-C' s against the elements given by F. B. Wood (I) in GCVS and by H. Rugemer (II) in SAC 38, respectively. Min = JD 2416426. 783+3.0633175d . E+0.021d . sin (0.09474deg . E+64.42deg) (I) Min = JD 2435584. 7500+3.0633175d. E (II) Our photoelectric observations are inconsistent with the remark in SAC 38, page 105 "A minimum recently observed by K. Kordylewski is in agreement with our ephemeris". The Nurnberg observations of TX UMa lead to the new elements: Min = JD 2438856.353 + 3.063243d. E (III) The minima obtained at the Nurnberg Observatory are given in the following Table together with the O-C' s computed with the formulas (I) to (III) Minima O-C (I) O-C (II) O-C (III) 2438856,354 -0.053d -0.019d +0.001d 39193,308 -0.067 -0.030 -0.002 39536,394 -0.076 -0.036 +0.001 Nurnberg Observatory E. POHL 85 Nurnberg, Lutzowstr. 10 Western Germany