Simple analytic formula relating the mass and spin of accreting compact objects to their rapid X-ray variability
Following the previous research on epicyclic oscillations of accretion disks around black holes (BHs) and neutron stars (NSs), a new model of high-frequency quasi-periodic oscillations (QPOs) has been proposed (CT model), which deals with oscillations of fluid in marginally overflowing accretion tor...
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Veröffentlicht in: | arXiv.org 2022-03 |
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Sprache: | eng |
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