activity
19962025
most citedEvolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945

1.6k citations · 17.4k across the 150 of their papers we have counts for

collaborators

143 papers

astro-ph.SR2025

Extreme Lithium Depletion in Solar Twins: Challenging Non-Standard Mixing Models

Isabelle Winnick, Jhon Yana Galarza, Henrique Reggiani +12

Lithium (Li) is a powerful tracer of stellar mixing, gradually depleted in solar twins by non-standard transport below the convective zone. Here, we identify six new solar twins wi…

physics.plasm-ph2025

Roadmap for warm dense matter physics

Jan Vorberger, Frank Graziani, David Riley +71

This roadmap presents the state-of-the-art, current challenges and near future developments anticipated in the thriving field of warm dense matter physics. Originating from strongl…

astro-ph.GA2024

JWST/NIRSpec Observations of Brown Dwarfs in the Orion Nebula Cluster

K. L. Luhman, C Alves de Oliveira, I. Baraffe +4

We have used the multiobject mode of the Near-Infrared Spectrograph (NIRSpec) on board the James Webb Space Telescope (JWST) to obtain low-resolution 1-5um spectra of 22 brown dwar…

astro-ph.SR2023

JWST/NIRSpec Observations of the Coldest Known Brown Dwarf

K. L. Luhman, P. Tremblin, C. Alves de Oliveira +6

We present 1-5um spectroscopy of the coldest known brown dwarf, WISE J085510.83-071442.5 (WISE 0855), performed with the Near-Infrared Spectrograph (NIRSpec) on board the James Web…

astro-ph.EP2023★ 11 cited

Evidence of Radius Inflation in Radiative GCM Models of WASP-76b due to the Advection of Potential Temperature

Felix Sainsbury-Martinez, Pascal Tremblin, Aaron David Schneider +6

Understanding the discrepancy between the radii of observed hot Jupiters and standard 'radiative-convective' models remains a hotly debated topic in the exoplanet community. One me…

astro-ph.SR2023★ 14 cited

Two-dimensional simulations of internal gravity waves in a 5 Zero-Age-Main-Sequence model

A. Le Saux, I. Baraffe, T. Guillet +5

Main-sequence intermediate-mass stars present a radiative envelope that supports internal gravity waves (IGWs). Excited at the boundary with the convective core, IGWs propagate tow…