Image Details
 
                    Caption: Fig. 4.
Pulse‐phase spectroscopy of 16 phase bins combined PCA and HEXTE data. The power‐law indices are shown for two assumed values of the relative normalization between the two detector types. The other nine phase bins are either nebular‐background or transition bins with too few net counts for useful spectroscopy.
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.