1998/03/23 by Jeroen Homan, J. Homan, M. van der Klis +6 · 1 citation
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #astro-ph
paper · pdf · doi:10.1086/311341
7 pages, 4 figures, accepted for publication in ApJ Letters
arxiv created 1998/03/23 · openalex publication_date 1998/05/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30
We report the discovery of a quasi-periodic oscillation (QPO) at 61.0 ± 1.7 Hz with the Rossi X-Ray Timing Explorer in the low-mass X-ray binary and persistently bright atoll source GX 13+1 (4U 1811-17). The QPO had an rms amplitude of 1.7% ± 0.2% (2-13.0 keV) and an FWHM of 15.9 ± 4.2 Hz. Its frequency increased with the count rate, and its amplitude increased with the photon energy. In addition, a peaked noise component was found with a cutoff frequency of ~2 Hz, a power-law index of around -4, and an rms amplitude of ~1.8%, probably the well-known atoll source high-frequency noise. It was found only when the QPO was detected. Very low frequency noise was present, with a power-law index of ~1 and an rms amplitude of ~4%. A second observation showed similar variability components. In the X-ray color-color diagram, the source did not trace out the usual banana branch but showed a two-branched structure. This is the first detection of a QPO in one of the four persistently bright atoll sources in the Galactic bulge. We argue that the QPO properties indicate that it is the same phenomenon as the horizontal-branch oscillations (HBOs) in Z sources. That HBOs might turn up in the persistently bright atoll sources was previously suggested on the basis of the magnetospheric beat-frequency model for HBOs. We discuss the properties of the new phenomenon within the framework of this model.