COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 582 Konkoly Observatory Budapest 1971 September 21 PHOTOELECTRIC AND SPECTROGRAPHIC OBSERVATIONS OF THE ECLIPSING VARIABLE SZ CAMELOPARDALIS The UBV photometry of the eclipsing variable SZ Camelopardalis (the northern component of BD+61d676) was carried out with the 36 inch reflectors at the Dodaira Station of Tokyo Astronomical Observatory and the Okayama Astrophysical Observatory on twenty-two clear nights during the winter of 1970-71. Some coude spectrograms were also taken with the 74 inch reflector at Okayama. [FIGURE 1] BD+61d669 was used as the primary comparison star in the photoelectric observations, which was the same one as used in the recent observation by Olsen (1971). The light of the southern component of BD+61d676 was observed occasionally for detection of its suspected small light variation (Guthnick and Prager 1930), but it was confirmed from our observations that the light of the southern component is constant within observational errors of the order of 0.004m - 0.006m. The figure shows our photoelectric light curve in B, where dots stand for observations with phases between 0 and 1/2 P and small circles for observations with phases between 1/2 P and P. We obtained the residual O-C=0.1052d for the primary minimum from Min. - JD 2427533.5191+ +2.6984166d E (Wesselink's ephemeris 1941). Therefore, the phases in the above figure were corrected by the value +0.1052d. This O-C value is in good agreement with Olsen's result from observation of the secondary minimum. 1971 September 13 M. KITAMURA and A. YAMASAKI Tokyo Astronomical Observatory, Mitaka, Tokyo References: Olsen, Erik Heyn 1971, IAU Bulletin of Commission 27, No. 533. [IBVS 533] Olsen, Erik Heyn 1971, June, private communication, Guthnik, P, and Prager, R. 1930, Astr. Nachrichten 239, 14. [BIBCODE 1930AN....239...13G ] Wesselink, A.J. 1941, Ann. Sterrew. Leiden 17, part 3. [BIBCODE 1941AnLei..17C...1W ]