Can disk-magnetosphere interaction models and beat frequency models for quasi-periodic oscillation in accreting X-ray pulsars be reconciled?

2008/11/01 by E. Bozzo, L. Stella, M. Vietri +1 · 4 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810658

11 pages, 3 figures. Accepted for publication on A&A

arxiv created 2008/11/01 · openalex publication_date 2008/12/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Aims. We review some aspects of the theory of magnetic threaded disks.

Citations

• Large X-Ray Flares from LMC X-4: Discovery of Millihertz Quasi-periodic Oscillations and Quasi-periodic Oscillation–Modulated Pulsations

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• Constraints on the disc–magnetosphere interaction in accreting pulsar 4U 1626−67