A. F. J. Moffat
Abstract
It is argued that the emission-line spectrum of the Large Magellanic Cloud (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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It is argued that the emission-line spectrum of the Large Magellanic Cloud (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
Key concepts: Wolf–Rayet star, Physics, Large Magellanic Cloud, Astrophysics, Nebula, Star (game theory), Astronomy, Stars