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The interaction of giant planets with a disc with MHD turbulence - III. Flow morphology and conditions for gap formation in local and global simulations

Monthly Notices of the Royal Astronomical Society, no. 3 (2004): 829-848

Cited: 85|Views27
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Abstract

We present the results of both global cylindrical disc simulations and local shearing box simulations of protoplanets interacting with a disc undergoing magnetohydrodynamic (MHD) turbulence with zero net flux magnetic fields. We investigate the nature of the disc response and conditions for gap formation. This issue is an important one fo...More

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