COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1675 Konkoly Observatory Budapest 1979 September 24 SEMIREGULAR 58 DAYS VARIATION IN VV Cep The long period eclipsing binary system VV Cep was observed on nearly 100 nights from August 1976 to September 1978 in the Red and Infrared colours. A preliminary analysis of the red plates, 103aE with RG1 filter, with a two minutes exposure at the focus of the 11 cm astrograph of the S. Vittore Observatory in Bologna, revealed a manifest semiregular variation with a period of approximately 58 days, as shown in Figure 1. Our period is about half of the period of 118 [FIGURE 1] Figure 1: moving averages on three plates. The mean error of each point is about 0.04 mag. days reported by McCook and Guinan (1978) based on Halpha photoelectric observations on 850 days, but with big intervals of straight 200 days. According to Hutchings and Wright (1971) these variations should come from the Halpha emission region with a radius of 150 R_Sun, surrounding the Be star, the eclipse of which should be partial. Red and Infrared observations are continued and we hope to observe before long the star also in Halpha. A complete analysis of the observations, including UBV photoelectric photometry of the eclipse, will be published elsewhere. We would like to thank Vacchi, Sassi and Sette for having done the observations till now and L. Baldeschi, A. Dalle donne, R. Di Luca, A. Ferri, C. Frisoni, G. Mengoli, A. Prosperi for helping in the reductions. L. BALDINELLI S. GHEDINI S. MARMI Osservatorio Astronomico "Guido Horn D'Arturo" C.P. 1630, 40100 Bologna A/D Italy References: Hutchings, J.B., Wright, K.O. 1971, M.N.R.A.S., 155, 203. [BIBCODE 1971MNRAS.155..203H ] McCook, G.P., Guinan, E.F. 1978, I.B.V.S., 1385