Image Details
Caption: Fig. 1.
Model spectra for different parameter values are shown together with the data from PI, corrected for interstellar absorption with ﹩N_{\mathrm{H}\,}=1.15\times 10^{20}﹩ cm−2 (see § 4). The model in the inset incorporates the effects of a warm absorber (see text for details).
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.