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Showing content from https://link.springer.com/article/10.12942/lrr-2014-3/figures/17 below:

Figure 17 | The Evolution of Compact Binary Star Systems

Estimates of regimes of mass transfer in WD binaries. Instantaneous tidal coupling is assumed. For longer time scales of tidal coupling, the stability limit in the plot shifts down [464]. The filled squares mark initial positions of the models studied in the quoted paper. Image reproduced with permission from [129], copyright by AAS.

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