COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3635 Konkoly Observatory Budapest 9 July 1991 HU ISSN 0374 - 0676 An improved, unambiguous period of the Ap star 108 Aqr The star 108 Aqr = HR 9031= HD 223640, classified B9pSiSrCr by Cowley et al. 1969, has been observed in the Geneva photometric system between 1986 and 1988 at ESO La Silla with the 70 cm Swiss telescope. The period (3.73 +- 0.03 days) published by Morrison & Wolff 1971, was not satisfactory because it was based on uvby measurements taken only once a night, so that the alias frequency 1-nu (i.e. P =1.37 days) was not excluded at all. Our 64 Geneva observations allow to exclude clearly the alias period (P =1.37 days), and our V data combined with the 36 y data of Morrison & Wolff 1971, yield the period P = 3.735236d +- 0.000024 while the maximum light in the V band occurs on HJD = 2444655.047. The resulting lightcurve is shown in Fig. 1, together with the fitted curve (a Fourier series truncated to the first harmonic). The r.m.s. residual scatter of all 100 V and y data together around the fitted curve is only 0.0042 magnitudes. [FIGURE 1] Figure 1: Lightcurve of 108 Aqr in the Geneva V band (crosses) and in Stromgren's y band (open dots). See the ephemeris in the text. P. North M. Burnet Institut d'astronomie Observatoire de Geneve de l'Universite de Lausanne ch. des Maillettes 51 CH-1290 Chavannes-des-Bois CH-1290 Sauverny Switzerland Switzerland References Cowley A., Cowley C., Jaschek M., Jaschek C., 1969, AJ. 74, 375 [BIBCODE 1969AJ.....74..375C ] Morrison N.D., Wolff S.C., 1971, PASP 83, 474 [BIBCODE 1971PASP...83..474M ]