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Cited article:

Variable Polarization of WR 31a: Binary Companion or Corotating Interaction Region?

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The Astronomical Journal 170 (1) 10 (2025)
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Optical Polarimetry of WR 1 Consistent with a CIR and 17 days Rotation

Nicolaus Steenken, Richard Ignace, Nicole St-Louis and Guillaume Lenoir-Craig
Research Notes of the AAS 9 (2) 36 (2025)
https://doi.org/10.3847/2515-5172/adb4ea

Rapid polarization variations in the O4 supergiant ζ Puppis

Jeremy Bailey, Ian D Howarth, Daniel V Cotton, Lucyna Kedziora-Chudczer, Ain De Horta, Sarah L Martell, Colin Eldridge and Paul Luckas
Monthly Notices of the Royal Astronomical Society 529 (1) 374 (2024)
https://doi.org/10.1093/mnras/stae548

Using CHIRON spectroscopy to test the hypothesis of a precessing orbit for the WN4 star EZ CMa

Krister D G Barclay, Sophie Rosu, Noel D Richardson, André-Nicolas Chené, Nicole St-Louis, Richard Ignace and Anthony F J Moffat
Monthly Notices of the Royal Astronomical Society 527 (2) 2198 (2023)
https://doi.org/10.1093/mnras/stad3289

Modelling variable linear polarization produced by Co-rotating Interaction Regions (CIRs) across optical recombination lines of Wolf–Rayet stars

R Ignace, J E Bjorkman, A-N Chené, C Erba, L Fabiani, A F J Moffat, R Sincennes and N St-Louis
Monthly Notices of the Royal Astronomical Society 526 (1) 1298 (2023)
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Monte Carlo simulations of polarimetric and light variability from corotating interaction regions in hot stellar winds

Danny Carlos-Leblanc, Nicole St-Louis, Jon E Bjorkman and Richard Ignace
Monthly Notices of the Royal Astronomical Society 489 (2) 2873 (2019)
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Polarization light curve modelling of corotating interaction regions in the wind of the Wolf–Rayet star WR 6

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Monthly Notices of the Royal Astronomical Society 474 (2) 1886 (2018)
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BRITE-Constellation high-precision time-dependent photometry of the early O-type supergiant ζ Puppis unveils the photospheric drivers of its small- and large-scale wind structures

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Searching for a magnetic field in Wolf–Rayet stars using FORS 2 spectropolarimetry

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Monthly Notices of the Royal Astronomical Society 458 (3) 3381 (2016)
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