COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1923 Konkoly Observatory Budapest 1981 February 11 HU ISSN 0374-0676 PHOTOELECTRIC MINIMA OF THE ECLIPSING BINARY PV CASSIOPEIAE The eclipsing binary PV Cas (BV 72; BD+58d2554) has been investigated by different authors (Geyer, 1961; Pohl, 1969; Ibanoglu, 1971, 1974) during the past twenty years. It was also observed photoelectrically at the Konkoly Observatory and four primary and seven secondary minima were obtained. BD+58d2562 was used as comparison star. The observations were made in B and V colours with the (*) 24" Newton telescope (in Budapest) equipped with an unrefrigerated EMI 9502 B photomultiplier and with the (**) 20" Cassegrain telescope (in the mountain station) equipped with an unrefrigerated EMI 9058 QB photomultiplier. The O-C values were calculated with the following elements given by Ibanoglu (1974) : Min I = J.D.Hel. 2440227.4044 + 1.75046986d E +- 3 +-16 Table I Times of minima Min. (Hel.) O-C Type Remark 2442233.4400 -0.0016 I ** 2716.5735 +0.0005 I ** 2766.4270 +0.0006 II * 2786.5905 -0.0005 I ** 2850.4495 +0.0006 II * 3046.5050 +0.0022 II * 3076.2635 +0.0025 II * 3125.2795 +0.0041 II * 3348.4910 -0.0007 I * 3482.3775 +0.0079 II * 3524,3860 +0.0038 II * J. KELEMEN Konkoly Observatory Budapest, Hungary References: Geyer, E.H.: Zeitschrift fur Astrophysik 51, 79 (1961) [BIBCODE 1961ZA.....51...79G ] Pohl, E.: Inf. Bull. Var. Stars No. 386 (1969) Ibanoglu, C.: Inf. Bull. Var. Stars No. 555 (1971) Ibanoglu, C.: Astronomy and Astrophysics, 35, 483 (1974) [BIBCODE 1974A&A....35..483I ]