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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. 1.

Snapshot of density and poloidal velocity vectors illustrating the jet and disk wind for all cases of disk density variation. Gray scale (logarithm of the number density measured in cm−3; ≤8.26 is white and ≥10.46 is black) and velocity scale are consistent for all frames. The panels, from top to bottom, are the low‐density case (at ﹩t=147﹩ days), the baseline case (at ﹩t=136﹩ days), and the high‐density case (at ﹩t=137﹩ days). In each panel, the equatorial plane is along the bottom, and the star is at bottom center.

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