Ec. Ford et al., Simultaneous measurements of X-ray luminosity and kilohertz quasi-periodicoscillations in low-mass X-ray binaries, ASTROPHYS J, 537(1), 2000, pp. 368-373
We measure simultaneously the properties of the energy spectra and the freq
uencies of the kilohertz quasi-periodic oscillations (QPOs) in 15 low-mass
X-ray binaries covering a wide range of X-ray luminosities. In each source,
the QPO frequencies cover the same range of approximately 300-1300 Hz, alt
hough the sources differ by 2 orders of magnitude in their X-ray luminositi
es (as measured from the unabsorbed 2-50 keV flux). So the X-ray luminosity
does not uniquely determine the QPO frequency. This is difficult to unders
tand since the evidence from individual sources indicates that the frequenc
y and luminosity are very well correlated at least over short timescales. P
erhaps beaming effects or bolometric corrections change the observed lumino
sities, or perhaps part of the energy in mass accretion is used to power ou
t 8ows, thus reducing the energy emitted in X-rays. It is also possible tha
t the parameters of a QPO model are tuned in such a way that the same range
of frequencies appears in all sources. Different modes of accretion may be
involved (for example, disk and radial), or multiple parameters may conspi
re to yield the same frequencies.