# Correction to: Effect of the rotation and tidal dissipation history of   stars on the evolution of close-in planets

**Authors:** Emeline Bolmont, St\'ephane Mathis

arXiv: 1902.01283 · 2019-02-13

## TL;DR

This paper corrects a previous study on how stellar rotation and tidal dissipation affect close-in planet evolution, and further explores the impact of planets on their host star's spin.

## Contribution

It provides a corrected analysis of stellar and planetary interactions, and investigates the influence of planets on stellar spin evolution.

## Key findings

- Corrected the spin integration in the previous model.
- Analyzed the influence of planets on host star spin.
- Enhanced understanding of star-planet tidal interactions.

## 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.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1902.01283/full.md

## References

7 references — full list in the complete paper: https://tomesphere.com/paper/1902.01283/full.md

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Source: https://tomesphere.com/paper/1902.01283