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Isabelle Baraffe
Researcher at University of Exeter
Publications - 295
Citations - 23718
Isabelle Baraffe is an academic researcher from University of Exeter. The author has contributed to research in topics: Brown dwarf & Stars. The author has an hindex of 72, co-authored 287 publications receiving 21612 citations. Previous affiliations of Isabelle Baraffe include University of Göttingen & University of Lyon.
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Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
TL;DR: In this article, the authors present evolutionary models for cool brown dwarfs and extra-solar giant planets and show that irradiation effects can substantially affect the radius of sub-jovian mass giant planets.
Journal ArticleDOI
Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945
TL;DR: In this article, the authors present evolutionary models for cool brown dwarfs and extra-solar giant planets and show that irradiation effects can substantially affect the radius of sub-jovian mass giant planets.
Journal ArticleDOI
New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
TL;DR: In this paper, the authors presented new models for low-mass stars down to the hydrogen-burning limit that consistently couple atmosphere and interior structures, thereby superseding the widely used BCAH98 models.
Journal ArticleDOI
New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
TL;DR: In this paper, the authors presented new models for low-mass stars down to the hydrogen-burning limit that consistently couple atmosphere and interior structures, thereby superseding the widely used BCAH98 models.
Journal ArticleDOI
Evolutionary Models for Very Low-Mass Stars and Brown Dwarfs with Dusty Atmospheres
Gilles Chabrier,Gilles Chabrier,Isabelle Baraffe,Isabelle Baraffe,F. Allard,Peter H. Hauschildt +5 more
TL;DR: In this paper, the interior of the most massive brown dwarfs is shown to develop a conductive core after ~2 Gyr which slows down their cooling, and the authors suggest the possibility of a brown dwarf dearth in J, H, and K color-magnitude diagrams around this temperature.