Fig. 4.

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Comparison of the tracks computed in the present study and the tracks computed using M − R relations, as in Nelemans et al. (2001a). The blue line represents the track for (MHe, 0 + MWD, 0, P0) = (0.43+0.87) M⊙, 90 min; the magenta line is the part of the track for the same system under the assumption of non-conservative mass exchange; and the cyan line represents the track for (MHe, 0 + MWD, 0, P0) = (0.33+0.72) M⊙, 35 min. Black dots mark RLOF. Green lines indicate the tracks computed using analytic M − R relations for the systems (MHe, 0 + MWD, 0, P0) = (0.33+0.72) M⊙, 35 min and (MHe, 0 + MWD, 0, P0) = (0.43+0.87) M⊙, 90 min (left to right, respectively). The black line is the LISA noise line, and the red line indicates the gravitational waves’ foreground+LISA noise.
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