[vsnet-alert 14754] Re: Spectroscopy of the Nova Sgr 2012 No.4

Thierry Garrel gabalou at gmail.com
Wed Jul 11 10:53:05 JST 2012


Spectroscopy of the Nova Sgr 2012 No.4

An echelle spectrum of the Nova Sgr No. 4 was taken on July 8.872 at a
resolution of R~11000 with a 0.35 schmidt cassegrain telescope at Fontcaude
observatory, Juvignac, France.

http://gabalou.canalblog.com/archives/2012/07/11/24681534.html

Thierry Garrel

2012/7/9 Christian Buil <christian.buil at wanadoo.fr>

> A spectrum of Nova Sgr No4 taken with LISA spectrograph at resolution of
> R=1000 and
> a 100 mm diameter refractor, only from France (Castanet observatory) :
>
> http://www.astrosurf.com/buil/**nova_sgr2012_4/obs.htm<http://www.astrosurf.com/buil/nova_sgr2012_4/obs.htm>
>
> Fe type nova.
> Date: July 8.962, 2012
> 3 x 300 sec. exposure.
>
> Christian Buil
>
>
>
>
> -----Message d'origine----- From: K. Imamura
> Sent: Sunday, July 08, 2012 8:36 PM
> To: vsnet-campaign-nova at ooruri.**kusastro.kyoto-u.ac.jp<vsnet-campaign-nova at ooruri.kusastro.kyoto-u.ac.jp>;
> vsnet-alert at ooruri.kusastro.**kyoto-u.ac.jp<vsnet-alert at ooruri.kusastro.kyoto-u.ac.jp>
> Subject: [vsnet-alert 14747] Spectroscopy of the Nova Sgr 2012 No.4
>
>
> Spectroscopy of the Nova Sgr 2012 No.4
>
>   We have obtained a spectrum (R~400) of the Nova Sgr 2012 No.4
> (CBET3166) on July 8.578 (UT), using the DSS-7 spectrometer
> attached to the 0.28-m Schmidt-Cassegrain telescope at the OUS
> Observatory. Emission lines of Balmer series, Fe II multiplets
> (27, 37, 38, 42, 46, 48, 49, 55 and 74), Na I D and O I (7773)
> can be seen in the spectrum. The FWHM of H-alpha is
> approximately 1800 km/s.
>
> Our spectra can be seen in the following:
>  http://tnblab.blog7.fc2.com/**blog-entry-319.html<http://tnblab.blog7.fc2.com/blog-entry-319.html>
>
> --
> Kazuyoshi Imamura (Okayama Univ. of Sci. team)
>


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