Fig. 2 from A New Instability of Accretion Disks around Magnetic Compact Stars

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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. 2.

Geometry of the reference systems of § 2.1. The K frame is inertial; its z axis is along the pulsar spin axis. The K^{﹩\arcmin﹩} frame rotates rigidly with the star; its z^{﹩\arcmin﹩} axis is aligned with the star's symmetry axis of its quadrupole moment.

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