Overview of tidal effects considered in this work, for stars with various internal structures. Convective envelopes may experience a combination of equilibrium tides from viscous dissipation, dynamical tides from IGW dissipation, and dynamical tides from IW dissipation. Boundaries between radiative and convective zones may excite dynamical tides from IGWs and IWs, which are dissipated in the radiative and convective zones of the star, respectively. In our models, convective cores do not experience tidal dissipation.