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1994PASP..106..626G - Publ. Astron. Soc. Pac., 106, 626-631 (1994/June-0)
A new ejecta shell surrounding a Wolf-Rayet star in the LMC.
GARNETT D.R. and CHU Y.-H.
Abstract (from CDS):
In contrast, the shell around Br 2 shows no clear evidence of enrichment. The nebular spectrum is characterized by extremely strong [O III] and He II emission and very weak [N II]. We derive normal He, O, and N abundances from our spectrum. This object therefore appears to be simply a wind-blown structure associated with a relatively dense cloud near the Wolf-Rayet star, although the very high ionization state of the gas is unusual for a nebula associated with a Wolf-Rayet star.
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Simbad objects: 6
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