activity
20132026
most citedSOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

273 citations · 1.9k across the 44 of their papers we have counts for

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astro-ph.EP2025

Modelling the effect of stellar metallicity on the XUV evolution of low-mass stars and its impact on exoplanet atmospheres/habitability

Victor See, Charlotte Fairman, Louis Amard +1

Understanding how exoplanet atmospheres evolve is a key question in the context of habitability. One key process governing this evolution is atmospheric evaporation by stellar X-ra…

astro-ph.EP2017★ 39 cited

Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets. II. Effect of stellar metallicity

Emeline Bolmont, Florian Gallet, Stéphane Mathis +3

Observations of hot Jupiter type exoplanets suggest that their orbital period distribution depends on the metallicity of their host star. We investigate here whether the impact of…

astro-ph.EP2017★ 82 cited

Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets I. From the PMS to the RGB at solar metallicity

Florian Gallet, Emeline Bolmont, Stéphane Mathis +2

Star-planet interactions must be taken into account in stellar models to understand the dynamical evolution of close-in planets. The dependence of the tidal interactions on the str…

astro-ph.EP2016

Effect of the rotation, tidal dissipation history and metallicity of stars on the evolution of close-in planets

Emeline Bolmont, Florian Gallet, Stéphane Mathis +2

Since 1995, numerous close-in planets have been discovered around low-mass stars (M to A-type stars). These systems are susceptible to be tidally evolving, in particular the dissip…

astro-ph.EP2016★ 52 cited

Impacts of stellar evolution and dynamics on the habitable zone: The role of rotation and magnetic activity

Florian Gallet, Corinne Charbonnel, Louis Amard +3

In this article, we aim to provide the community with the dependence of the habitable zone upon the stellar mass, metallicity, rotation, and for various prescriptions of the limits…

astro-ph.EP2015★ 273 cited

SOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

A. Santerne, C. Moutou, M. Tsantaki +19

While giant extrasolar planets have been studied for more than two decades now, there are still some open questions such as their dominant formation and migration process, as well…