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[en] Spectrophotometric observations of two remarkably faint WR stars in the LMC show them to be heavily reddened Population I stars. The brighter is a normal WC4 star but the fainter is a WN3-4 star with exceptionally strong emission lines, especially C IVlambda5806 which is of a strength equal to that found in WC stars. (author)
Journal
Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; 
; CODEN MNRAA; v. 224(2); p. 435-442
; CODEN MNRAA; v. 224(2); p. 435-442