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[vsnet-history 20] EY Cyg + Nova Sgr 1992 + V1017 Sgr (Schmeer)

Date: Thu, 24 Apr 2003 10:37:13 +0900 (JST)
To: vsnet-history@ooruri.kusastro.kyoto-u.ac.jp
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
Subject: [vsnet-history 20] EY Cyg + Nova Sgr 1992 + V1017 Sgr (Schmeer)
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From: Patrick Schmeer
To  : Taichi Kato
Date: 1992-04-07

Dear Taichi,

many thanks for your 2 recent e-mails.

EY CYGNI  (UGSS:)
May it be too late to detect superhumps in EY Cyg (at least 10
days after maximum)?
Will you try to take a wide field CCD frame of this DN? 
Is the difference between comparison stars '108' and '115'
really 0.7 magnitudes? Perhaps you could check the field visually.
I would be interested in V magnitudes of stars 110, 118, 122, 125,
131, 137 on the AAVSO chart.

NOVA SAGITTARII 1992, V1017 SAGITTARII
How bright are these 2 stars currently?

Kind regards,
Patrick

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