VLA observations of WR 147 and HD 167971 yield no detectable linear radio polarization above roughly 1 percent, attributed to turbulent magnetic fields, Faraday rotation, beam depolarization, and thermal dilution from stellar winds.
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Search for radio polarization in the particle-accelerating colliding-wind binaries WR 147 and HD 167971
VLA observations of WR 147 and HD 167971 yield no detectable linear radio polarization above roughly 1 percent, attributed to turbulent magnetic fields, Faraday rotation, beam depolarization, and thermal dilution from stellar winds.