Image Details
Caption: Fig. 1.
Phase residuals for the accretion‐powered pulsations (bars; red) and the burst oscillations (crosses; blue), compared to a model that has a constant frequency and orbital Doppler shifts. The final burst, which has no detectable first‐overtone component, requires special treatment; see text. The units on the right axis are rotational cycles. The top panel shows the outburst light curve.
© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.