[vsnet-alert 8554] Nova Sgr 2005 No.2: spectrum by Fujii

Taichi Kato tkato at kusastro.kyoto-u.ac.jp
Thu Jul 7 12:30:18 JST 2005


   M. Fujii (Fujii Bisei Observatory) took a spectrum
of Nova Sgr 2005 No.2 on July 6.59 UT:

   http://www1.harenet.ne.jp/~aikow/etc/nova_sgr_no2_20050706.gif

   The balmer series emission lines are strong (FWHM of Halpha
= 1900km/s).  The Fe II-series emission lines are also present.
The spectrum is a typical one for an Fe II-class nova.


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