We review the current state of knowledge of magnetic fields inside stars, concentrating on
recent developments concerning magnetic fields in stably stratified (zones of) stars, leaving …

We study tidal dissipation in stars with masses in the range 0.1–1.6 M⊙ throughout their
evolution, including turbulent effective viscosity acting on equilibrium tides and inertial …

Warm Jupiters lay out an excellent laboratory for testing models of planet formation and
migration. Their separation from the host star makes tidal reprocessing of their orbits …

Observations of hot Jupiters around solar-type stars with very short orbital periods (∼ 1 d)
suggest that tidal dissipation in such stars is not too efficient so that these planets can …

A large fraction of known exoplanets have short orbital periods where tidal excitation of
gravity waves within the host star causes the planets' orbits to decay. We study the effects of …

We study the orbital evolution of hot Jupiters due to the excitation and damping of tidally
driven g-modes within solar-type host stars. Linearly resonant g-modes (the dynamical tide) …

We study the excitation and damping of tides in close binary systems, accounting for the
leading-order nonlinear corrections to linear tidal theory. These nonlinear corrections …

We study tidal dissipation in hot Jupiter host stars due to the nonlinear damping of tidally
driven g-modes, extending the calculations of Essick & Weinberg to a wide variety of stellar …

Magnetic interactions between a star and a close-in planet are postulated to be a source of
enhanced emissions and to play a role in the secular evolution of the orbital system. Close …

In compact white dwarf (WD) binary systems (with periods ranging from minutes to hours),
dynamical tides involving the excitation and dissipation of gravity waves play a dominant …