COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1285 Konkoly Observatory Budapest 1977 May 27 ON THE PERIOD OF SW Lac SW Lac is one of the well observed W UMa-type stars. The average lengths of period of this star were given by Purgathofer and Prohazka (1966): Table 1 Years Period Change of DeltaP period 1893-1914 0.3207124d 1914-1928 0.3207151 JD 2419990 +0.23s 1928-1951 0.3207166 2425210 +0.13 1951-1960 0.3207213 2433690 +0.41 1960-1968 0.3207282 2436755 +0.60 ------------------------------------------------- 1973- 0.3207144 -1.19 It can be seen from Table 1 and from the O-C curve (Fig. 1) that the period was increasing in the years 1893-1968. The analysis of the photoelectric times of minima from the years 1969- 1976 leeds to the conclusion that the period of SW Lac decreased 1.2 sec in the years 1969-1973. The possible reason of this decrease of the period may be: 1. The O-C curve has a periodical nature with a period of about 80 years and the changes in the period of SW Lac might be due to the existence of a third component, as it was mentioned by Schilt (1923) - but there is no evidence for a third body in this system. 2. The changes of period are attributed to the instrinsic variability of SW Lac, mainly to the active mass exchange processes in the system. Further photoelectric observations of this interesting system and determinations of times of minima would be highly desirable. [FIGURE 1] Predictions of times of minima for the near future are given by the formula: Min. I =JD 244 2697.404 + 0.3207144d E. ZOFIA FRASINSKA J.M. KREINER Astronomical Observatory Silesian University of the Jagiellonian Institute of Physics University Astronomical Laboratory Cracow, Poland Katowice, Poland References: Purgathofer, A., Prohazka, F. 1966 Mitt. Wien 13, 151 Schilt, J. 1923 B.A.N. 2, 1 [BIBCODE 1923BAN.....2....1S ]