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Simulations, Data Analysis and Algorithms

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Figure 2 | Computational Astrophysics and Cosmology

Figure 2

From: On the origin of jets from disc-accreting magnetized stars

Figure 2

Two-component outflows observed in slowly (left) and rapidly (right) rotating magnetized stars. The background shows the poloidal matter flux F m =ρ v p , the arrows are the poloidal velocity vectors, and the lines are sample magnetic field lines. The labels point to the main outflow components. In the left-hand panel α ν =0.3 and α η =0.3 while in the right-hand panel α ν =0.1= α η .

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