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Paper: Modeling the Colliding Wind Spectra of CV Ser (WR 113)
Volume: 465, Four Decades of Massive Star Research - A Scientific Meeting in Honor of Anthony J. Moffat
Page: 351
Authors: Hill, G. M.; Moffat, A. F. J.; St-Louis, N.
Abstract: High S/N, moderate resolution spectra of the 29.7 d WC8 + OB binary CV Ser (WR 113) which provide full phase coverage have been obtained. These data show variations of the C III λ5696 emission line profile typical of those seen in WR + OB colliding wind systems. Preliminary modeling is presented based on code we have used for other, similar systems.
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