A New Instability of Accretion Disks around Magnetic Compact Stars
Authors: Mario Vietri and Luigi Stella
Vietri &
Stella
1998 The Astrophysical Journal503350.
Provider: AAS Journals
Caption: Fig. 1.
Geometry of the blob–magnetic field interaction. The two panels correspond to different phases of the blob orbital evolution, showing that the acceleration along the z axis (eq. [1]) alternates in sign.