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[vsnet-obs 45239] SY Sco V407 Sco Bright Maximum
- Date: Tue, 27 May 2003 07:03:35 +1000
- To: "vsnet-lpv" <vsnet-lpv@ooruri.kusastro.kyoto-u.ac.jp>,"vsnet-chat" <vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp>
- From: "Peter F Williams" <pfwilliams@onaustralia.com.au>
- Subject: [vsnet-obs 45239] SY Sco V407 Sco Bright Maximum
- Cc: "vsnet-obs" <vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp>
- Delivered-To: vsnet-obs-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
- Reply-To: <pfwilliams@onaustralia.com.au>
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
Two of the brighter Mira type variables in line of sight with the open
cluster Messier 7 are currently near maximum and well placed for
observation in this very attractive field. Both are somewhat brighter than
the GCVS listed maximum as per the following recent observations. Please
enjoy.
SCOSY 20030301.764 <140 WPX
SCOSY 20030502.536 102 WPX
SCOSY 20030521.492 93 WPX
SCOV407 20030301.763 <140 WPX
SCOV407 20030502.536 140 WPX
SCOV407 20030521.491 109 WPX
Regards
Peter Williams
Heathcote NSW
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