Image Details
Caption: Figure 5.
Exponents α of the best power-law fits to the power spectra of the light curves as functions of
(horizontal axis) and inclination angle (vertical axis). The departures from α ≈ −2 in the upper-right-hand corner of the
plot are caused by the disk's self-obscuration. The black curves represent contours of
R
o
. From bottom to top,
.
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