Dear colleagues, We have submitted the following article to IAUC. Regards, Daisaku Nogami and Taichi Kato ------------------------------------------------------------------ >From nogami Tue Apr 18 05:03:55 1995 To: GREEN@CFA.HARVARD.EDU, MARSDEN@CFA.HARVARD.EDU Cc: nogami, tkato Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION I would like to submit the following article to IAUC. Best regards, Daisaku Nogami and Taichi Kato Dept. of Astronomy, Kyoto University Apr. 17 1995 ============ AL COMAE BERENICES The V-band CCD photometry obtained by a 0.60-m reflector at Ouda Station, Kyoto University, indicate that the hump-like feature reported independently by J. Patterson and J. A. DeYoung (IAUC 6157) showed a continous decay until Apr. 12. The data between Apr. 17.440 UT and 17.691 UT clearly demonstrate a periodic modulation with a period of 0.0576 +/- 0.0002 day, and with an amplitude of 0.18 mag. This period is slightly longer than those reported earlier and one (0.05666 +/- 0.00002 day) determined by us from Apr. 7 - 12 observations. This fact indicates that the new features are genuine superhumps, and earlier detection may reflect a variation related to the orbital motion of the underlying binary. The present observation thus first firmly identifies the SU UMa-type nature of AL Com. However, the base-line is not so long. The follow-up observations are expected.