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NICIL: A Stand Alone Library to Self-Consistently Calculate Non-Ideal Magnetohydrodynamic Coefficients in Molecular Cloud Cores

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RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR COLLAPSE: PROTOSTELLAR CORE FORMATION

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MODELING THE RESOLVED DISK AROUND THE CLASS 0 PROTOSTAR L1527

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DOES MAGNETIC-FIELD-ROTATION MISALIGNMENT SOLVE THE MAGNETIC BRAKING CATASTROPHE IN PROTOSTELLAR DISK FORMATION?

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A ∼0.2-solar-mass protostar with a Keplerian disk in the very young L1527 IRS system

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Bridging the gap: disk formation in the Class 0 phase with ambipolar diffusion and Ohmic dissipation

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INCORPORATING AMBIPOLAR AND OHMIC DIFFUSION IN THE AMR MHD CODE RAMSES

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THE ROLE OF TURBULENT MAGNETIC RECONNECTION IN THE FORMATION OF ROTATIONALLY SUPPORTED PROTOSTELLAR DISKS

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Small-scale properties of low-mass Class 0 protostars: digging into the memory of accretion processes

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Magnetic fields during the early stages of massive star formation - I. Accretion and disc evolution

D. Seifried, R. Banerjee, R. S. Klessen, D. Duffin and R. E. Pudritz
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NON-IDEAL MHD EFFECTS AND MAGNETIC BRAKING CATASTROPHE IN PROTOSTELLAR DISK FORMATION

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DISK FORMATION IN MAGNETIZED CLOUDS ENABLED BY THE HALL EFFECT

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Magnetic Diffusion in Star Formation

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EXPOSED LONG-LIFETIME FIRST CORE: A NEW MODEL OF FIRST CORES BASED ON RADIATION HYDRODYNAMICS

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