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A new Wolf-Rayet star in the Small Magellanic Cloud
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1991
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PhotometryEngineeringO-star Absorption SpectrumSmall Magellanic CloudStellar StructureAstronomical Image AnalysisAstrophysical PlasmaNew Wolf-rayet StarSynchrotron RadiationAstrophysicsNew Wr Star
A new WR star in the Small Magellanic Cloud identified on a UK Schmidt Telescope objective prism plate is found to be similar in character to other SMC WR stars in that it has weak emission lines plus an O-star absorption spectrum. It is classified as WN2.5 + O5:.