[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 6294] Re: New eclipsing star in the OU Vir field?
- Date: Mon, 05 May 2003 13:02:56 -0700
- To: Daisaku NOGAMI <nogami@kwasan.kyoto-u.ac.jp>
- From: Arne Henden <aah@nofs.navy.mil>
- Subject: [vsnet-chat 6294] Re: New eclipsing star in the OU Vir field?
- Cc: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- References: <20030506015754P.nogami@kwasan.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.0.1) Gecko/20021003
I just looked at Bruce Sumner's 1999 sequence for this field; he
has the eclipsing variable mentioned, along with four
datapoints showing the variability. The sequence can be found
at either my anon ftp site or at Mike Simonsen's site:
http://joevp.20m.com/charts/henden/Her%20to%20Vul/
The new variable is already marked on Mike's charts. So its
variability has been known, just not published by itself.
Arne
Daisaku NOGAMI wrote:
> Dear colleagues,
>
> The star USNO B1.0 0892-0239905 (14 34 43.0780, -00 47 10.230
> (J2000.0)), which is one of the check stars in our OU Vir data,
> is showing an eclipse-like modulation. Is this a new eclipsing
> variable?
>
> Best regards,
> Daisaku Nogami
>
>

Return to Home Page

Return to the Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology