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The Origin of Massive Stars: The Inertial-inflow Model
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Modeling the Accretion Disk around the High-mass Protostar GGD 27-MM1
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A new hybrid radiative transfer method for massive star formation
Salt, Hot Water, and Silicon Compounds Tracing Massive Twin Disks
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Gravity and Rotation Drag the Magnetic Field in High-mass Star Formation
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Population synthesis of exocometary gas around A stars
Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
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Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H ii regions – spherically symmetric ionized accretion flows
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Driving conditions of protostellar outflows in different star-forming environments
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Fragmentation, rotation, and outflows in the high-mass star-forming region IRAS 23033+5951
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