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Magnetic Fields in the Infrared Dark Cloud G34.43+0.24
UploadALMA Reveals Sequential High-mass Star Formation in the G9.62+0.19 Complex
UploadAmbipolar Diffusion Heating in Turbulent Systems
UploadComparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
UploadPhotoionization Rates in Clumpy Molecular Clouds
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