COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3122 Konkoly Observatory Budapest 22 December 1987 HU ISSN 0374-0676 A NEW VARIABLE STAR IN CASSIOPEIA In an observational program on the eclipsing binary AB Cas, BD + 70 188 was used as the comparison star (also used by Ando, 1980) and SAO 4710 (BD+70 199= HD 16439) as the check star. The observations showed that while BD + 70 188 kept a nearly constant brightness, SAO 4710 presented an undoubted photometric variability. This last star is not present in any of the variable star catalogues, hence it has to be considered as a new variable star. SAO 4710 was observed three nights in November 1987 with the 75 cm reflector at the "Sierra Nevada" Observatory (Spain) in the Stromgren four colours. Figure 1 shows the light curve in the v filter for November 17 th. In a preliminary Fourier [FIGURE 1] Figure 1. - Light curve in the v filter at November 17th, with E = SAO 4710 and C1 = BD +70 188. The magnitudes are in the instrumental system. analysis of these light curves we could verify that SAO 4710 is a monoperiodic pulsator with an amplitude of 0.041 mag in the v filter. After prewhitening of the main frequency (17.1438 c/d) the power spectrum does not show any further peak with a global amplitude greater than 0.007 A tentative ephemeris is given as: HJD max. = 2447117.39742 + 0.05833d E +/-8 +/-5 The general aspect of the light curves suggests that we are dealing with a Delta Scuti type variable. A more detailed study of this star will be published later. J.L. SEDANO E. RODRIGUEZ P. LOPEZ DE COCA Instituto de Astrofisica de Andalucia Apdo. 2144, Granada, Spain Reference: Ando, H. 1980, Astrophys. Space Sci. 71, 249. [BIBCODE 1980Ap&SS..71..249A ]