185 citations · 594 across the 9 of their papers we have counts for
12 papers
TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars
C. Moutou, J. M. Almenara, G. Hébrard +40
We present the discovery of two new transiting extrasolar planet candidates identified as TOI-1296.01 and TOI-1298.01 by the Transiting Exoplanet Survey Satellite (TESS). The plane…
A new equation of state for dense hydrogen-helium mixtures II: taking into account hydrogen-helium interactions
Gilles Chabrier, Florian Debras
In a recent paper (Chabrier et al. 2019), we have derived a new equation of state (EOS) for dense hydrogen/helium mixtures which covers the temperature-density domain from solar-ty…
Superadiabaticity in Jupiter and giant planet interiors
F. Debras, G. Chabrier, D. Stevenson
Interior models of giant planets traditionally assume that at a given radius (i.e. pressure) the density should be larger than or equal to the one corresponding to a homogeneous, a…
Observational signatures of eccentric Jupiters inside gas cavities in protoplanetary discs
Clément Baruteau, Gaylor Wafflard-Fernandez, Romane Le Gal +4
Predicting how a young planet shapes the gas and dust emission of its parent disc is key to constraining the presence of unseen planets in protoplanetary disc observations. We inve…
Revisiting migration in a disc cavity to explain the high eccentricities of warm Jupiters
F. Debras, C. Baruteau, J. -F. Donati
The distribution of eccentricities of warm giant exoplanets is commonly explained through planet--planet interactions, although no physically sound argument favours the ubiquity of…
Idealised simulations of the deep atmosphere of hot jupiters: Deep, hot, adiabats as a robust solution to the radius inflation problem
F. Sainsbury-Martinez, P. Wang, S. Fromang +10
Context: The anomalously large radii of hot Jupiters has long been a mystery. However, by combining both theoretical arguments and 2D models, a recent study has suggested that the…