Fig. 3 from Simulation‐based Investigation of a Model for the Interaction between Stellar Magnetospheres and Circumstellar Accretion Disks

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Simulation‐based Investigation of a Model for the Interaction between Stellar Magnetospheres and Circumstellar Accretion Disks

Authors: Sean Matt, Anthony P. Goodson, Robert M. Winglee, and Karl-Heinz Böhm

Matt et al. 2002 The Astrophysical Journal 574 232.

Provider: AAS Journals

Caption: Fig. 3.

Same as Fig. 1 but for truncated disk (at ﹩t=143﹩ days), open magnetosphere (at ﹩t=138﹩ days), and closed magnetosphere cases (at ﹩t=145﹩ days). The insets in each panel show the magnetic field topologies at the start of the simulation (at a smaller scale; star is at lower left).

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