Figure 12 from Bipolar Jets Launched by a Mean-field Accretion Disk Dynamo

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Bipolar Jets Launched by a Mean-field Accretion Disk Dynamo

Authors: Christian Fendt, and Dennis Gaßmann

2018 The Astrophysical Journal 855 130.

Provider: AAS Journals

Caption: Figure 12.

Time evolution of the mass fluxes for different strengths of the dynamo α₀. The mass fluxes are calculated at (accretion) or within (ejection) R = 3, respectively. Thus the most powerful inner part of the jet is considered.

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