The Effect of Misalignment between the Rotation Axis and Magnetic Field on the Circumstellar Disk

The formation of circumstellar disks is investigated using three-dimensional resistive magnetohydrodynamic simulations in which the initial prestellar cloud has a misaligned rotation axis with respect to the magnetic field. We examine the effects of (i) the initial angle difference between the globa...

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Veröffentlicht in:The Astrophysical journal 2020-08, Vol.898 (2), p.118
Hauptverfasser: Hirano, Shingo, Tsukamoto, Yusuke, Basu, Shantanu, Machida, Masahiro N.
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Sprache:eng
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