Correction to: Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets
arXiv:1902.01283 · doi:10.1007/s10569-018-9880-2
Abstract
This is an erratum for the publication Bolmont & Mathis 2016 (Celestial Mechanics and Dynamical Astronomy, 126, 275-296, https://doi.org/10.1007/s10569-016-9690-3). There was a small mistake for the spin integration of our code which we corrected and we take advantage of this erratum to investigate a bit further the influence of a planet on the spin of its host star.
This erratum was accepted for publication in Celestial Mechanics and Dynamical Astronomy. 6 pages, 3 figures