COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3539 Konkoly Observatory Budapest 8 November 1990 HU ISSN 0374 - 0676 An independent confirmation of rapid oscillations in the cool Ap star HD 12932 The V=10.3 Ap star HD 12932 is classified as Ap SrEuCr by Houk and Smith-Moore (1988), making it a good candidate for rapid oscillations. Weiss and Schneider 1990 (private communication and I.B.V.S., submitted) have just discovered it to be a rapidly oscillating Ap (roAp) star; in this bulletin, I report an independent confirmation of the detection of rapid oscillations. Photometry was obtained on three nights in Oct. 1990 with the Lowell 1.1-m John S. Hall telescope and the 0.8-m reflector in Johnson B. A total of over 7 hours of photometry was obtained over a time-span of 7 days. A periodicity analysis of the data was undertaken utilizing Kurtz' (1985) faster algorithm of the Deeming (1975) DFT technique. The figure shows a peak in the amplitude spectrum near 124 c/d (nu=1.44 mHz), corresponding to a period of about 11.6 minutes. A least-squares cosine fit to the data yields a best fit to the period 11.605+/-0.003 minutes, with a semi-amplitude of 2.27 millimagnitudes. I gratefully acknowledge the Lowell Observatory endowment for support of this research. [FIGURE 1] TOBIAS J. KREIDL Lowell Observatory Mars Hill Rd., 1400 West Flagstaff, AZ 86001, U.S.A. References: Deeming, T.J., 1975. Astrophys. Space Sci., 36, 137. [BIBCODE 1975Ap&SS..36..137D ] Houk, N., Smith-Moore, M., 1988. Michigan Spectral Catalogue, Vol. 4, Department of Astronomy, University of Michigan, Ann Arbor. [BIBCODE 1988mcts.book.....H ] Kurtz, D.W., 1985. Mon. Not. R. astr. Soc., 213, 773. [BIBCODE 1985MNRAS.213..773K ] * The discovery note has been published by Schneider and Weiss in the No. 3520 issue of the I.B.V.S. (Editors). [IBVS 3520]