Image Details
Caption: Figure 7.
Left: periodogram of the frequency variations of 4U1608-522 as derived from the MLEs of the QPO frequency on a timescale of
16 s. The best power-law fit is shown with a dashed line (index 1.8 ± 0.2). Right: broadening of the QPO with increasing integration
time of the fitted PDS. As expected from a random walk, the broadening goes like
. The best fit is shown with a dot-dashed line. Such analysis enables us to derive the intrinsic QPO width to be 3.2 Hz, corresponding
to a quality factor of 259 ± 5 at a frequency of 829 Hz.
© 2012. The American Astronomical Society. All rights reserved.