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

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

Author(s) -

Shoji Kato

Publication year - 2005

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/57.3.l17

Subject(s) - physics , precession , astrophysics , neutron star , resonance (particle physics) , low mass , black hole (networking) , quasi periodic , astronomy , stars , atomic physics , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol

We try to understand the quasi-periodic oscillations (QPOs) in low-massneutron-star and black-hole X-ray binaries by a resonance model in warped diskswith precession. Our main concern is high-frequency QPOs, hectohertz QPOs, andhorizontal-branch QPOs in the z sources and the atoll sources, and thecorreponding QPOs in black-hole X-ray binaries. Our resonance model canqualitatively, but systematically, explain these QPOs by regarding hectohertzQPOs as a precession of warp.Comment: 4 pages, to be published in PASJ Vol.57, No.

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