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[vsnet-alert 120] the submitted article on AL Com
- Date: Tue, 18 Apr 1995 15:10:44 +0900
- To: vsnet-alert@sanma.kusastro.kyoto-u.ac.jp
- From: Daisaku Nogami <nogami@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 120] the submitted article on AL Com
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.
Return to Daisaku Nogami
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