Bipolar planetary nebulae from common-envelope evolution of binary stars

Open Access

Fig. A.3.

(Movie online) Movie of the launching of the bipolar outflow. Similar to Fig. 5, we show the evolution of gas density, the absolute magnetic-field strength (|B|), the radial velocity (v_rad), and the ratio of magnetic to thermal pressure (β⁻¹) perpendicular to the orbital plane.

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