Resonance model for high-frequency QPOs in white dwarfs, neutron stars and black holes

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

High-frequency QPOs reflect non-linear, and likely resonant,
oscillations in accretion disks. In black holes, and probably in neutron
stars, but not in white dwarfs, strong gravity plays a crucial role in
their formation.

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