Evolution of angular-momentum-losing exoplanetary systems

2014/11/27 by C. Damiani, A. F. Lanza · 1 citation
Physics and Astronomy · #Angular momentum #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Classical mechanics #Exoplanet #Hot Jupiter #Physics #Planet #Planetary system #Population #Stars #Stellar, planetary, and galactic studies #Tidal acceleration #astro-ph.EP #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201424318

published as A&A 574, A39 (2015) · 22 pages, 11 figures, accepted for publication in A&A

openalex publication_date 2014/11/27 · arxiv created 2014/11/30 · arxiv updated 2015/01/28 · openalex created_date 2019/12/26 · openalex updated_date 2026/07/31

Abstract

Aims. We assess the importance of tidal evolution and its interplay with magnetic braking in the population of hot-Jupiter planetary systems.

Citations

• Fast Tides in Slow Stars: The Efficiency of Eddy Viscosity
• On the Origins of Eccentric Close-In Planets
• COUPLING THE SOLAR DYNAMO AND THE CORONA: WIND PROPERTIES, MASS, AND MOMENTUM LOSSES DURING AN ACTIVITY CYCLE
• Tidal Dissipation in Rotating Solar‐Type Stars
• SOPHIE velocimetry ofKeplertransit candidates
• Tidal dissipation in binary systems
• OBSERVATIONAL EVIDENCE FOR TIDAL DESTRUCTION OF EXOPLANETS
• The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets
• Tidal Evolution of Close‐in Extrasolar Planets

Cited by

• An Eccentric Brown Dwarf Eclipsing an M dwarf