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The role of magnetic fields in the formation of high-mass star-forming cores
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Filamentary mass accretion towards the high-mass protobinary system G11.92–0.61 MM2
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Fragmentation of the High-mass “Starless” Core G10.21-0.31: A Coherent Evolutionary Picture for Star Formation
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A Massive Star Is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
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