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| Paper: |
Large-Scale Structures in Wolf-Rayet Winds: Single vs Binary |
| Volume: |
367, Massive Stars in Interactive Binaries |
| Page: |
117 |
| Authors: |
Chene, A.-N.; St.-Louis, N. |
| Abstract: |
Spectroscopic monitoring of a large number of presumably single WR stars is revealing a significant number that display large-scale line-profile variability (LSLPV). In those cases where periods are found but no evidence of a binary companion, we believe that we are seeing evidence of rotation of the underlying star. The monitoring of this LSLVP may be a unique opportunity to measure the rotation rate of Wolf-Rayet stars which is still, until now, generally unknown. |
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