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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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 2years
2026 2representative citing papers
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
citing papers explorer
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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.
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Long-term optical variability of high-mass X-ray binaries. III. Polarimetry
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.