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Home All issues A&A, 423 2 (2004) 693-704 Article references

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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

Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain

Kenneth G. Gayley, Jorick S. Vink, Asif ud-Doula, et al.
Astrophysics and Space Science 367 (12) (2022)
https://doi.org/10.1007/s10509-022-04142-6

Radio variability from corotating interaction regions threading Wolf–Rayet winds

Richard Ignace, Nicole St-Louis and Raman K Prinja
Monthly Notices of the Royal Astronomical Society 497 (1) 1127 (2020)
https://doi.org/10.1093/mnras/staa2014

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

Investigating the origin of cyclical wind variability in hot massive stars – II. Hydrodynamical simulations of corotating interaction regions using realistic spot parameters for the O giant ξ Persei

A. David-Uraz, S. P. Owocki, G. A. Wade, J. O. Sundqvist and N. D. Kee
Monthly Notices of the Royal Astronomical Society 470 (3) 3672 (2017)
https://doi.org/10.1093/mnras/stx1478

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

S. Hubrig, K. Scholz, W.-R. Hamann, et al.
Monthly Notices of the Royal Astronomical Society 458 (3) 3381 (2016)
https://doi.org/10.1093/mnras/stw558

Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics

U. M. Noebauer and S. A. Sim
Monthly Notices of the Royal Astronomical Society 453 (3) 3121 (2015)
https://doi.org/10.1093/mnras/stv1849

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

THE Hα VARIATIONS OF THE LUMINOUS BLUE VARIABLE P CYGNI: DISCRETE ABSORPTION COMPONENTS AND THE SHORT S DORADUS-PHASE

N. D. Richardson, N. D. Morrison, D. R. Gies, et al.
The Astronomical Journal 141 (4) 120 (2011)
https://doi.org/10.1088/0004-6256/141/4/120

THE THREE-DIMENSIONAL MORPHOLOGY OF A COROTATING INTERACTION REGION IN THE INNER HELIOSPHERE

B. E. Wood, R. A. Howard, A. Thernisien and D. G. Socker
The Astrophysical Journal 708 (2) L89 (2010)
https://doi.org/10.1088/2041-8205/708/2/L89

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

Looking for Discrete UV Absorption Features in the Early‐Type Eclipsing Binariesμ1Scorpii and AO Cassiopeiae

M. L. Arias, J. Sahade, H. F. Henrichs and Y. Kondo
Publications of the Astronomical Society of the Pacific 117 (833) 730 (2005)
https://doi.org/10.1086/431267