2005/10/24 by W. Kluźniak, Wlodek Kluzniak
Physics and Astronomy · #Astrophysical Phenomena and Observations #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.1002/asna.200510420
published as Astron.Nachr.326:820-823,2005
openalex publication_date 2005/10/24 · arxiv created 2005/10/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Abstract Some of the more promising ideas about the origin of the high frequency variability (kHz QPOs) in the observed X‐ray emissions of low‐mass X‐ray binaries are contrasted with less promising ones. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)