A WC9 subclass Wolf-Rayet star in the Large Magellanic Cloud?

Details A WC9 subclass Wolf-Rayet star in the Large Magellanic Cloud? A WC9 subclass Wolf-Rayet star in the Large Magellanic Cloud?

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244l...9m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 1, April 1991, p. L9, L10. NSERC-supported research.

Astronomy and Astrophysics

Astrophysics

16

Early Stars, H Ii Regions, Interstellar Matter, Magellanic Clouds, Wolf-Rayet Stars, Astronomical Spectroscopy, Carbon, Emission Spectra, Nitrogen, Oxygen, Stellar Composition

Scientific paper

It is argued that the emission-line spectrum of the LMC nebula N82 with
embedded star(s) probably does not contain a WC9 spectrum, as claimed
previously. A WNL or Of type spectrum appears more likely. Thus, the low
WC content of the LMC remains as before: completely dominated by WCE
stars.

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