Fig. 12 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. 12.

Squares and dotted lines are as in Fig. 4 but for disk oscillation period at ﹩t=160﹩ days. The triangles represent a semianalytical calculation (see text).

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