COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2597 Konkoly Observatory Budapest 1 October 1984 HU ISSN 0374-0676 TIMES OF MAXIMUM LIGHT OF THE BETA CMa STAR BW VULPECULAE An extensive study of the times of maximum light of BW Vul was carried out by Valtier (1976). In it he considers all the available photometric and spectroscopic data in view of the importance of establishing rates of period increase for comparison with theoretical models of the stars. Valtier finds that, in agreement with Cherewick and Young (1975), all the observations can be fitted by a unique ephemeris if one considers that the period is linearly increasing with a rate of 1.8 s/century. In view of the importance of this result, some additional observations were carried out at the Observatorio Jose Arbol y Bonilla, Zacatecas, Mexico, with the 50 cm. telescope in the UBV system with a 1P21 uncooled phototube. The comparison stars were HD 199102 and HD 198527, except in 1982 when HD 198820 and HD 198527 were utilized. Table I lists the new times of maximum light for BW Vulpeculae. The photometric data and the analysis of periodicity will be published elsewhere. Table I Times of maximum light of BW Vulpeculae H.J.D. H.J.D. H.J.D. 44117.7225 44153.7070 44475.7782 44142.6620 44155.7220 44500.7160 44143.6560 44157.7378 44505.7409 44144.6560 44159.7490 45230.6945 44146.6773 44163.5651 45231.6977 44149.6950 Acknowledgement. Two of us (MRH and MRB) would like to thank Dr. T. Jarzebowski for suggesting the observations of this star. M. RIOS HERRERA (1), M. RIOS BERUMEN (1), J.H. PENA (2) and R. PENICHE (2) 1 Universidad Autonoma de Zacatecas, Apdo. Postal 275, Zacatecas, Zac., Mexico 2 Instituto de Astronomia Universidad Nacional Autonoma de Mexico Apdo. Postal 70-624, 04510 Mexico, D.F. Mexico References: Cherewick, T.A., and Young, A., 1975, Publ. Astron. Soc. Pacific, 87, 311. [BIBCODE 1975PASP...87..311C ] Valtier, J.C., 1976, Astron. Astrophys., 51, 465. [BIBCODE 1976A&A....51..465V ]