COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2757 Konkoly Observatory Budapest 9 July 1985 HU ISSN 0374 - 0676 ON THE MEAN CYCLE-LENGTH OF THE U GEMINORUM STAR VW VULPECULAE VW Vul has been suspected by Shafter (Inf.Bull.Variable Stars No. 2373 and Astron.J. 90, 643) as being a U Geminorum star of SU Ursae Majoris type; he also gave an estimate of the mean cycle-length of "roughly 30 days" (according to Mattei, unpublished). Since its discovery by Wolf in 1904 (Astron.Nachr. 166, 77) and a few estimates given by him (Astron.Nachr. 221, 261; 1924) no long-term photometric observations have been published. Its probable nature as a cataclysmic variable was not detected before 1978, when Bond (Publ.Astron.Soc.Pac. 90, 526) found spectroscopic features. I therefore determined the brightness of VW Vul on 132 Sonneberg plates taken with the 140/700 mm Triplet camera between 1930 and 1969 by the late R. Brandt. On this material the star varied from 13.1m to>14.9m pg., exhibiting the numerous "bright observations" typical for a medium-cycle U Geminorum star: 27 observations show the star in the upper part of the eruptions down to 0.6 mag below maximum light. At this level an average width of 4d+/-1d of the outbursts can be deduced from the short series of the AFOEV (observer Verdenet, Bull. 26; 27a-28; 30). With this, our material statistically yields a mean cycle-length of about 19d+/-5d. That means that the findings of Mattei and the AFOEV, from a comparatively very short time interval, are confirmed by our 40 years' data, thus indicating a stable behaviour of the star. W. WENZEL Sternwarte Sonneberg Zentralinstitut fur Astrophysik der Akademie der Wissenschaften der DDR