Fig. 9 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. 9.

Radial location of the inner edge of the accretion disk as a function of time (solid line), sensitive to variations in the disk mass. The three panels correspond to three cases with different initial disk densities, and the dashed line in each is the location of the Keplerian corotation point.

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