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

ASTRONOMY & ASTROPHYSICS, (2012)

Cited by: 75|Views3

Abstract

Context. Ideal magnetohydrodynamical (MHD) simulations have revealed catastrophic magnetic braking in the protostellar phase, which prevents the formation of a centrifugal disk around a nascent protostar. Aims. We determine if non-ideal MHD, including the effects of ambipolar diffusion and Ohmic dissipation determined from a detailed chem...More

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