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[vsnet-j 2413] V463 Sct
- Date: Tue, 26 Nov 2002 19:27:17 +0900 (JST)
- To: vsnet-j@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-j 2413] V463 Sct
- Sender: owner-vsnet-j@ooruri.kusastro.kyoto-u.ac.jp
V463 Sct について、以下のようなコメントをもらいました。T Pyx と光度曲線が
似ているかも知れないとのことです。将来もモニターする意義があるかも知れま
せん。また昔の写真を調べてみることも意義があるかも知れません。
Date: Tue, 26 Nov 2002 12:11:55 +0200 (EET)
From: "A.E. Rosenbush" <mijush@MAO.Kiev.UA>
Dear Dr.Kato,
recently I reviewed my "library" and I pay my attention to
your paper on the interpretation of V463 Sct (Nova Scuty 2000).
I think there is one more possibilty to relate this interesting
star to the T Pyx type recurrent novae, i.e. it is a recurrent nova
with the pre-nova about 19-20 mag.
It is a variable star therefore it is absent on DDS images.
I think a simiarity of light curves in the logarithmic time is
a good indication for other similarities.
Sincerely yours,
Alexander Rosenbush
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