Two faint WR stars near 30 Doradus

Details Two faint WR stars near 30 Doradus Two faint WR stars near 30 Doradus

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.224..435m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 224, Jan. 15, 1987, p. 435-442.

Astronomy and Astrophysics

Astronomy

17

Hydrogen Clouds, Magellanic Clouds, Stellar Luminosity, Stellar Spectrophotometry, Wolf-Rayet Stars, Carbon Stars, Emission Spectra, Interstellar Extinction, Line Spectra

Scientific paper

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 IV λ5806 which is of a
strength equal to that found in WC stars.

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