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2009CBET.1995....1K - Central Bureau Electronic Telegrams, 1995, 1 (2009/October-0)
Nova Sagittarii 2009 no. 4.
KINUGASA K., HONDA S., HASHIMOTO O., TAGUCHI H. and TAKAHASHI H.
Abstract (from CDS):
K. Kinugasa, S. Honda, O. Hashimoto, H. Taguchi and H. Takahashi, Gunma Astronomical Observatory (GAO), write that a low-resolution spectrum (range 420-800 nm; resolution 1.0 nm), obtained with the GAO 1.5-m telescope (+ GLOWS) on Oct. 27.4 UT, confirms that the object announced on CBET 1994 is a nova, showing H_alpha emission (FWHM about 600 km/s) with a P-Cyg profile, its absorption minimum being blue-shifted by 900 km/s with respect to the emission peak. Fe II (multiplet 42) lines also have P-Cyg profiles.
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