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Cited article:

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XMM–Newton X-ray observations of the Wolf–Rayet binary system WR 147

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A Steady, Radiative‐Shock Method for Computing X‐Ray Emission from Colliding Stellar Winds in Close, Massive‐Star Binaries

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High-resolution X-ray imaging of the colliding wind shock in WR 147 (WN8(h)+B0.5V)

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