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Using Shell models to investigate clumping in the wind of the O7Iaf + supergiant AzV83

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Advances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directions

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Chandra grating spectroscopy of embedded wind shock X-ray emission from O stars shows low plasma temperatures and significant wind absorption

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X-ray emission from BH+O star binaries expected to descend from the observed galactic WR+O binaries

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New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars

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