output
20042026
most citedA comparative study of disc-planet interaction

446 citations

Showing 2016 · astro-ph.EPShow all

9 papers · 2 filters

astro-ph.EP2016★ 32 cited

Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems

Amaury H. M. J. Triaud, Marion Neveu-VanMalle, Monika Lendl +16

We report the detection of two new systems containing transiting planets. Both were identified by WASP as worthy transiting planet candidates. Radial-velocity observations quickly…

astro-ph.EP2016★ 74 cited

A Machine Learns to Predict the Stability of Tightly Packed Planetary Systems

Daniel Tamayo, Ari Silburt, Diana Valencia +9

The requirement that planetary systems be dynamically stable is often used to vet new discoveries or set limits on unconstrained masses or orbital elements. This is typically carri…

astro-ph.EP2016★ 35 cited

Disentangling Hot Jupiters formation location from their chemical composition

Mohamad Ali-Dib

We use a population synthesis model that includes pebbles and gas accretion, planetary migration, and a simplified chemistry scheme to study the formation of hot-Jupiters. Models h…

astro-ph.EP2016★ 36 cited

Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars

Veselin B. Kostov, Keavin Moore, Daniel Tamayo +2

Inspired by the recent Kepler discoveries of circumbinary planets orbiting nine close binary stars, we explore the fate of the former as the latter evolve off the main sequence. We…

astro-ph.EP2016★ 26 cited

A pebbles accretion model with chemistry and implications for the solar system

Mohamad Ali-Dib

We investigate the chemical composition of the solar system's giant planets atmospheres using a physical formation model with chemistry. The model incorporate disk evolution, pebbl…

astro-ph.EP2016★ 91 cited

Rossiter--McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems

D. J. A. Brown, A. H. M. J. Triaud, A. P. Doyle +12

We present new measurements of the projected spin--orbit angle for six WASP hot Jupiters, four of which are new to the literature (WASP-61, -62, -76, and -78), and two of which…