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Fig. 2

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Initial and final clump masses, denoted as Mcl and Mf, as well as the gap opening mass Mgap in our fiducial system NN Ser with model parameters αM = 1.1, αL = 12.5, and n = 1 in the absence of radiative feedback. The final clump masses are close to the gap opening mass scale, implying that they can evacuate the orbit and therefore ensure their survival.

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