Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay
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DOI: 10.1093/mnras/staa2405
Abstract: We study tidal dissipation in stars with masses in the range $0.1-1.6 M_\odot$ throughout their evolution, including turbulent effective viscosity acting on equilibrium tides and inertial waves in convection zones, and internal gravity waves in… read more here.
Keywords: orbital decay; mass; planetary orbital; dissipation ... See more keywords