[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 291] Re: CH Cyg
- Date: Thu, 8 May 1997 17:30:22 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-chat 291] Re: CH Cyg
- Cc: gp@star.sr.bham.ac.uk
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Gary Poyner wrote in [vsnet-chat 236]:
> Although the light variations of CH Cyg are well reported on VSNET, little
> is said about eclipses in this system. As a visual observer I would be
> very interested to know if anyone has observed these visually in the past,
> and our chances of monitoring them in the future!
According to Hinkle et al. 1993 (AJ 105, 1074), the spectroscopic
conjunction of the suggested 756-day binary (inner binary) occurs
JDconj = 2446643.655 + 756.0 * E
(red giant in front).
The conjunction times correspond to the following epochs.
JD
24446644 1986 Jul. - Aug.
47400 1988 Aug.
48156 1990 Sep.
48912 1992 Oct.
49667 1994 Nov.
50423 1996 Dec.
Looking back through visual observations from the AFOEV and VSOLJ
records, I could only find possible hints of fadings in the latest two
moments. CH Cyg showed a shallow minimum between 1994 Nov. and 1995
Jan.; in 1996 the star showed its historical minimum around July. The
association of these visual fadings with eclipses still needs to be
verified.
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp