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2009IAUC.9089....2K - IAU Circ., 9089, 2 (2009/October-0)
V5584 Sagittarii = 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 this variable star 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.
Abstract Copyright: ∼
Journal keyword(s):
Status at CDS : Objects in title, abstract, text, figures, and all or part of small table(s) being processed in SIMBAD.
Simbad objects: 1
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