Fig. 1
Evolution of the orbital period (solid curve) and the donor star mass (dashed curve) vs. evolutive timescale for LMXB. LMXB has a donor star with an initial mass of 1.5 M⊙ and an initial orbital period of 2.57 d. Horizontal dotted lines on the bottom of the figure correspond to the observed mass of WD with its error, and horizontal dotted line on the top of the figure represents the observed orbital period.
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