First observation of a transition between "parallel tracks" in the kHz QPO frequency vs. intensity diagram
| dc.creator | Mendez, Mariano | |
| dc.date | 2002-07-12 | |
| dc.date.accessioned | 2026-07-07T02:04:18Z | |
| dc.date.available | 2026-07-07T02:04:18Z | |
| dc.description | Contrary to theoretical expectations, observations with the Rossi X-ray Timing Explorer (RXTE) show that in X-ray binaries timing properties are not uniquely correlated with X-ray luminosity. For instance, although the frequencies of the kilohertz quasi-periodic oscillations (kHz QPOs) correlate with X-ray flux on short (~few hours) time scales, on time scales longer than a day the QPO appears at more or less the same frequency, whereas the luminosity may be a factor of a few different. The result is a set of almost parallel tracks in a QPO frequency vs. X-ray flux plot. Despite the "parallel tracks" are a common phenomenon among kHz QPO sources, until now, after five years of observations with RXTE, not a single transition between two of these tracks had been seen. Here I present the first detection of such a transition, in 4U 1636-53. | |
| dc.description | 2 pages, 1 figure, to appear in the Jan van Paradijs Memorial Symposium, eds. E.P.J. van den Heuvel, L. Kaper and E. Rol; Astronomical Society of the Pacific | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207279 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207279 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4698 | |
| dc.subject | Astrophysics | |
| dc.title | First observation of a transition between "parallel tracks" in the kHz QPO frequency vs. intensity diagram | |
| dc.type | text |