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- W3101235807 abstract "Relativistic Lense–Thirring precession of a tilted inner accretion disk around a compact object has been proposed as a mechanism for low-frequency (∼0.01–70 Hz) quasi-periodic oscillations (QPOs) in the light curves of X-ray binaries. A substantial misalignment angle (∼15°–20°) between the inner-disk rotation axis and the compact-object spin axis is required for the effects of this precession to produce observable modulations in the X-ray light curve. A consequence of this misalignment is that in high-inclination X-ray binaries the precessing inner disk will quasi-periodically intercept our line of sight to the compact object. In the case of neutron-star systems, this should have a significant observational effect, since a large fraction of the accretion energy is released on or near the neutron-star surface. In this Letter, I suggest that this specific effect of Lense–Thirring precession may already have been observed as ∼1 Hz QPOs in several dipping/eclipsing neutron-star X-ray binaries." @default.
- W3101235807 created "2020-11-23" @default.
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- W3101235807 date "2012-11-08" @default.
- W3101235807 modified "2023-10-16" @default.
- W3101235807 title "A POSSIBLE SIGNATURE OF LENSE-THIRRING PRECESSION IN DIPPING AND ECLIPSING NEUTRON-STAR LOW-MASS X-RAY BINARIES" @default.
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- W3101235807 doi "https://doi.org/10.1088/2041-8205/760/2/l30" @default.
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