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Cited article:

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Mass-loss Rates for O and Early B Stars Powering Bow Shock Nebulae: Evidence for Bistability Behavior

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The Astronomical Journal 158 (2) 73 (2019)
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Demonstration of a Novel Method for Measuring Mass-loss Rates for Massive Stars

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X-ray, UV and optical analysis of supergiants: ϵ Ori

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No breakdown of the radiatively driven wind theory in low-metallicity environments★†

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Line-driven winds and the UV turnover in AGN accretion discs

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