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Fig. 10


Orbital evolution of 1 MJ planets with different initial semi-major axes around NGC 4349 No. 127 (upper panel) and NGC 2423 No. 3 (lower panel). The green dashed lines show planets that will be engulfed during RGB, while blue pointed lines show the tracks of planets engulfed after the He-burning phase. The evolution of stellar radius is shown with a red line.

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