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Cited article:

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

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

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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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