| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780161 | New Astronomy Reviews | 2008 | 5 Pages |
Abstract
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.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Włodzimierz Kluźniak,