The Kepler space mission has discovered about a dozen planets orbiting around binary
stars systems. Most of these circumbinary planets lie near their instability boundaries, at …

We present an extended version of the Constant Time Lag analytical approach for the tidal
evolution of circumbinary planets introduced in our previous work. The model is self …

Most confirmed circumbinary planets are located very close to their host binary where the
tidal forces are expected to play an important role in their dynamics. Here we consider the …

We present a tidal model for treating the rotational evolution in the general three-body
problem with arbitrary viscosities, in which all the masses are considered to be extended …

We simulate the coupled stellar and tidal evolution of short-period binary stars (orbital period
P orb≲ 8 days) to investigate the orbital oscillations, instellation cycles, and orbital stability of …

Tidal evolution of low-eccentric circumbinary planets is expected to drive the rotational
evolution toward a pseudo-synchronous solution. In this work, we present a study of the …

En los últimos años se han descubierto muchos planetas presumiblemente rocosos, con
masas entre 1 y 10 M⊕, y que describen órbitas muy cercanas a su estrella anfitriona …