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Coherence of Burst Oscillations and Accretion‐Powered Pulsations in the Accreting Millisecond Pulsar XTE J1814−338

  • Authors: Anna L. Watts, Alessandro Patruno, and Michiel van der Klis

Watts, Patruno, & van der Klis 2008 The Astrophysical Journal Letters 688 L37.

  • Provider: AAS Journals

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.

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