COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 138 Konkoly Observatory Budapest 9 June 1966 PHOTOELECTRIC OBSERVATIONS OF THE NEW DELTA SCUTI VARIABLE HD 107904 HD 107904 (F0) belonging to the Hyades moving group was suggested by O. J. Eggen to be a delta Scuti-variable. From 22 spectra taken with the 36" Yapp reflector D. H. P. Jones and C. M. Haslam (The Observatory 86, 34, 1966) derived a radial velocity curve of about 30 km/sec amplitude and a period of 0.1707d -typical for a delta Scuti- variable. A first series of photoelectric b, v observations with the 24" reflector of the Lippert Astrograph (1966 May) covering a whole period show the respective light variation (figure). The comparison star used was BD +43deg2221 of spectral type F2, for which star preliminary measurements give V = 7.098m and B-V = 0.369m in the B, V system. The ordinates in the figure give the magnitude differences Delta b = b^0_var-b^0_comp and Delta v = v^0_var-v^0_com in the instrumental system. The color B-V refers to the B, V system. As it was an extraordinary photometric night the mean error of one observation turned out to be about +/-0.002m. As yet photoelectric measurements have been made in 4 nights yielding the following results: Maximum Delta m_b^max ampl._b Delta m_v^max ampl._v 243 9247.4423 -1.156m 0.150m -1.127m 0.110m 9259.5075: -1.070 0.029 -1.067 0.019 9262.4850 -1.100 0.065 -1.095 0.047 9266.4129 -1.111 0.056 -1.096 0.044 [FIGURE 1] It is known that variations in form and amplitude of the light curve are quite usual for delta Scuti variables. Further observations are urgently needed to get at the secondary period of these variations. 1966 May 29 A. A. WACHMANN Hamburg Bergedorf Sternwarte