[vsnet-chat 1210] Re: V592 Her: examination of the 1986 outburst data (schmeer)

[Taichi Kato <tkato>]

From extpasc@rz.uni-sb.de Sat Aug 29 18:42 JST 1998
From: Patrick Schmeer <extpasc@rz.uni-sb.de>
Subject: Re: [vsnet-chat 1208] Re: V592 Her: examination of the 1986 outburst data
To: tkato@kusastro.kyoto-u.ac.jp (Taichi Kato)
Date: Sat, 29 Aug 1998 11:42:42 +0200 (CST)
Cc: extpasc@rz.uni-sb.de (Patrick Schmeer)
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> I caught the EY Cyg outburst of the same year (independent detection) using
Dear Taichi,
 
> the same instrument, when the variable was reported below mag 13 or even
> below 14 by several AAVSO observers.  I included in my "list for 10-cm
Then you should have been able to see EY Cyg at minimum (about mag 14.7).
 
You must have had a very good sky. I can see mag 14.5 stars with my 20-cm
telescope only under very good conditions (there are, however, quite a lot of
streetlights around).
 
> 
>    Best question to ask!  Good candidates (range are from literatures, which
> might easily be superseded by future observations) are PQ And (8.8 mag),
> LS And (8.5 mag), UZ Boo (9.0 mag), VX For (>9.5 mag!), GW Lib (9.5 mag,
> maybe slightly smaller), V4338 Sgr (>12 mag?) and to name some.
> 
Do you have more information about VX For (max/min brightness, outburst dates)? 
V4338 Sgr = Nova Sgr 1990, isn't it? How probable is the DN classification?
 
Best regards,
Patrick

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