Fig. 3 from Eclipse Timings of the Low‐Mass X‐Ray Binary EXO 0748−676. III. Orbital Period Jitter Observed with the Unconventional Stellar Aspect Experiment and the Rossi X‐Ray Timing Explorer

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Eclipse Timings of the Low‐Mass X‐Ray Binary EXO 0748−676. III. Orbital Period Jitter Observed with the Unconventional Stellar Aspect Experiment and the Rossi X‐Ray Timing Explorer

Authors: Michael T. Wolff, Paul Hertz, Kent S. Wood, Paul S. Ray, and Reba M. Bandyopadhyay

Wolff et al. 2002 The Astrophysical Journal 575 384.

Provider: AAS Journals

Caption: Fig. 3.

Difference in the ﹩O{\mbox{﹩-﹩}} C﹩ residuals for the case of consecutive observed eclipse cycles. We plot here ﹩( O{\mbox{﹩-﹩}} C) _{n}-( O{\mbox{﹩-﹩}} C) _{n-1}﹩ when the observed eclipse cycle number n increases by 1.

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