Fig. 2.
(a) Pulse periods of X Persei determined every 70 d with the MAXI/GSC. The colors specify different values of Porb employed to correct the pulse arrival times for the orbital motion of the NS. (b) Pulse-period residuals, obtained from panel (a) by subtracting a linear trend and folding at the assumed Porb.

(a) Pulse periods of X Persei determined every 70 d with the MAXI/GSC. The colors specify different values of Porb employed to correct the pulse arrival times for the orbital motion of the NS. (b) Pulse-period residuals, obtained from panel (a) by subtracting a linear trend and folding at the assumed Porb.

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