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Fig. 8

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Survival chart of a 1.0 MIo satellite for different satellite dissipations, from no dissipation (top row) to Δtsat = 1.0 Δt (bottom row), and for equilibrium tide only (Col. 1) and dynamical tide (Cols. 2-4) for different initial stellar rotation periods: 1 day (Cols. 1-2), 3 day (Col. 3) and 8 day (Col. 4). The fate of the satellites is a function of the disk lifetime (left vertical axis) and the corresponding final semimajor axis of the planet (right vertical axis) and its initial position (horizontal axis). The red and blue regions correspond to where the satellite is disrupted, and the green region to where it can survive. The black dashed line shows the final planet semimajor axis below which there is no survival of the satellites. The crossed-out area corresponds to cases where the planet itself falls onto the star.

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