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Cited article:

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)
https://doi.org/10.1093/mnras/stad2878

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)
https://doi.org/10.1093/mnras/stz2273

Polarization light curve modelling of corotating interaction regions in the wind of the Wolf–Rayet star WR 6

N. St-Louis, Patrick Tremblay and Richard Ignace
Monthly Notices of the Royal Astronomical Society 474 (2) 1886 (2018)
https://doi.org/10.1093/mnras/stx2813

Long-wavelength, free–free spectral energy distributions from porous stellar winds

R. Ignace
Monthly Notices of the Royal Astronomical Society 457 (4) 4123 (2016)
https://doi.org/10.1093/mnras/stw216

Polarimetric modeling of corotating interaction regions threading massive-star winds

Richard Ignace, Nicole St-Louis and Félix Proulx-Giraldeau
Astronomy & Astrophysics 575 A129 (2015)
https://doi.org/10.1051/0004-6361/201424806

Modeling Ultraviolet Wind Line Variability in Massive Hot Stars

A. Lobel and R. Blomme
The Astrophysical Journal 678 (1) 408 (2008)
https://doi.org/10.1086/529129

Kinematic model inversions of hot star recurrent DAC data – tests against dynamical CIR models

J. Krtička, R. K. Barrett, J. C. Brown and S. P. Owocki
Astronomy & Astrophysics 417 (3) 1039 (2004)
https://doi.org/10.1051/0004-6361:20034372