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1998A&A...338L..91P - Astronomy and Astrophysics, volume 338L91-94 (1998/10-3)
The identification of the star SPH2 as a new WN4 star with strong CIV.
PEREIRA C.B., MACHADO M.A.D., LANDABERRY S.J.C. and DA CONCEICAO F.
Abstract (from CDS):
We report spectroscopic observations of a new Wolf-Rayet star not identified yet. This star is located in our Galaxy, in the Canis Majoris region and was discovered during a southern spectroscopic survey of stars previously identified as Hα emission objects. The star, SPH 2, after Schwartz, Persson & Hamann (SPH) (1990AJ....100..793S), shows the main characteristics of a WN star and a strong CIV 5808 typical of a WC star. Here, we present some of the main spectroscopic features and discuss a possible subtype classification. We also present line intensities and equivalent widths of the identified transitions.
Abstract Copyright: ∼
Journal keyword(s): Wolf-Rayet: general - Wolf-Rayet: WN stars - emission line stars
Simbad objects: 1
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