Tidal Dissipation in Rotating Low-Mass Stars and Implications for the Orbital Evolution of Close-In Massive Planets

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201730662
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Effect of the Stellar Spin History on the Tidal Evolution of Close-In Planets

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Tidal Dissipation and the Formation ofKeplernear-resonant Planets

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Deformation and Tidal Evolution of Close-In Planets and Satellites Using a Maxwell Viscoelastic Rheology

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Non-Standard S-Process in Low Metallicity Massive Rotating Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Massive Stars in the Local Group: Implications for Stellar Evolution and Star Formation

Annual Review of Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Terrestrial Planets and Water Delivery Around Low-Mass Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Evolution of Massive Stars With Rotation and Mass Loss

Symposium - International Astronomical Union
2004English

The Role of Rotation and Mass Loss in the Evolution of Massive Stars

Symposium - International Astronomical Union
2003English

The Snow Line in Viscous Disks Around Low-Mass Stars: Implications for Water Delivery to Terrestrial Planets in the Habitable Zone

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2015English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy