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On the nature of the WO3 star DR1 in IC 1613

We present the results of a quantitative spectroscopic analysis of the oxygen-sequence Wolf- Rayet star DR1 in the low-metallicity galaxy IC 1613. Our models suggest that the strong oxygen emission lines are the result of the high temperature of this WO3 star and do not necessarily reflect a more advanced evolutionary stage than WC stars.

preprint2013arXivOpen access
F. TramperG. GräfenerO. E. HartoogH. SanaA. de KoterJ. S. VinkL. E. EllerbroekN. LangerM. GarciaL. KaperS. E. de Mink
astro-ph.SR
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Open access11 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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F. TramperG. GräfenerO. E. HartoogH. SanaA. de KoterJ. S. VinkL. E. EllerbroekN. LangerM. GarciaL. KaperS. E. de Mink

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