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[vsnet-j 2298] Re: Nova Sgr 2002 (No. 3): spectroscopic confirmation by Mitsugu Fujii
- Date: Sun, 22 Sep 2002 11:46:10 +0900 (JST)
- To: dgreen@cfa.harvard.edu, vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@ooruri.kusastro.kyoto-u.ac.jp, vsnet-discovery-nova@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-j 2298] Re: Nova Sgr 2002 (No. 3): spectroscopic confirmation by Mitsugu Fujii
- Cc: khaseda@mx1.tees.ne.jp, vsnet-j@ooruri.kusastro.kyoto-u.ac.jp, vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-j@ooruri.kusastro.kyoto-u.ac.jp
Re: Nova Sgr 2002 (No. 3): spectroscopic confirmation by Mitsugu Fujii
> Mitsugu Fujii (Fujii Bisei Observatory, Okayama, Japan) reports
> (via K. Ayani, Bisei Astronomical Observatory) the spectrum of Haseda's
> new object taken on 2002 Sep. 21.44 UT. The object shows strong Balmer
> and Fe II emission lines. The FWHM of Halpha emission is 2400 km/s.
> This observation confirms that the object is an Fe II-class nova shortly
> after maximum.
Fujii communicates that the spectrum can be seen at:
http://vsnet1.harenet.ne.jp/~aikow/nova_sgr_no3.gif
(Averaged spectrum -- the mean time of the observation is different from
the initial report)
Regards,
Taichi Kato
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