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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Pith papers citing it
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2026 2representative citing papers
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.
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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A new wideband radio polarization observation of the Supernova Remnant G315.4$-$2.3
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.