A Resonance Model of Quasi-Periodic Oscillations of Low-Mass X-Ray Binaries

Details A Resonance Model of Quasi-Periodic Oscillations of Low-Mass X-Ray Binaries A Resonance Model of Quasi-Periodic Oscillations of Low-Mass X-Ray Binaries

2005-05-11

arxiv.org/abs/astro-ph/0505215v1

Astronomy and Astrophysics

Astrophysics

4 pages, to be published in PASJ Vol.57, No.3

Scientific paper

We try to understand the quasi-periodic oscillations (QPOs) in low-mass neutron-star and black-hole X-ray binaries by a resonance model in warped disks with precession. Our main concern is high-frequency QPOs, hectohertz QPOs, and horizontal-branch QPOs in the z sources and the atoll sources, and the correponding QPOs in black-hole X-ray binaries. Our resonance model can qualitatively, but systematically, explain these QPOs by regarding hectohertz QPOs as a precession of warp.

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