Image Details
Caption: Fig. 4.
Power spectra and fit functions in the power spectral density times frequency representation. Each plot corresponds to a different region in the CCDs and color‐intensity diagrams (see Figs. 1 and 2). The curves mark the individual Lorentzian components of the fit. For detailed identification, see Table 3 and Fig. 5.
© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.