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Quasi-Periodic Oscillations: The Rapid Burster (MXB 1730-335): Models vs. Observations - A Brief Review
Published online by Cambridge University Press: 04 August 2017
Abstract
The salient features of quasi-periodic oscillations (QPO) observed in type 2 bursts and in the persistent emission from the Rapid Burster are discussed. In addition, a brief review is given of the models that have recently been proposed to explain high-frequency QPO observed in several bright low-mass X-ray binaries. We do not yet know the mechanism(s) of the QPO, not even whether they are magnetospheric in origin. However, some of the proposed ideas could well be relevant to the various rather complex aspects of the QPO. It is likely that more than one mechanism is at work.
- Type
- IV. Neutron Stellar Evolution
- Information
- Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 363 - 374
- Copyright
- Copyright © Reidel 1987