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A New Instability of Accretion Disks around Magnetic Compact Stars

  • Authors: Mario Vietri and Luigi Stella

Vietri & Stella 1998 The Astrophysical Journal 503 350.

  • 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.

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