A star's response to losing up to 10 percent of its mass depends mainly on its mass: stars above about 0.7 solar masses become denser and more resistant to further stripping, while lower-mass stars become less dense and more fragile, and tidal heating is negligible in both cases.
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Repeated Tidal Interactions between Stars and Supermassive Black Holes: Mass Transfer, Stability, and Implications for Repeating Partial Tidal Disruption Events
A star's response to losing up to 10 percent of its mass depends mainly on its mass: stars above about 0.7 solar masses become denser and more resistant to further stripping, while lower-mass stars become less dense and more fragile, and tidal heating is negligible in both cases.