Results 261 to 270 of about 10,374 (277)

Early Evolution of Planets in Binaries: Planet–Disk Interaction

2010
Among the extrasolar planetary systems detected over 30 are located in a stellar binary orbiting one of the stars, preferably the more massive primary. The dynamical influence of the second companion alters firstly the orbital elements of the forming protoplanet directly and secondly the structure of the disk from which the planet formed. The latter in
Willy Kley, Richard P. Nelson
openaire   +1 more source

Planet-disk interactions in the AB Aurigae system: revisiting the hypothetical vortex

I] ContextStructures and asymmetries detected in protoplanetary disks offer an exciting means to characterize the orbital and physical properties of embedded proto-planets, which are suspected to sculpt some of the observed features. A dozen of young disks have been reported to harbor crescent-shaped dust rings at millimeter wavelengths, with compact ...
Thomas Collin-Dufresne, Emmanuel Di Folco, Arnaud Pierens   +2 more
openaire   +1 more source

Gas disk interactions, tides and relativistic effects in the rocky planet formation at the substellar mass limit

Astronomy and Astrophysics, 2022
Mariana B Sanchez, G C De Elía
exaly  

Planet-disk interaction in solar system analogs: looking for planets and substructures in debris disk systems.

Debris disks represent the final phase in protoplanetary disk evolution. As byproducts of planet formation, these disks typically contain planetesimal belts, dust, and gas. Similar to our own solar system's debris disk, planetary systems often create inner dust clearing through gravitational interactions.Understanding the relationship between planets ...
Veronica Roccatagliata, Min Kim
openaire   +1 more source

Planet-disk interaction: eccentricity excitation and orbital evolution

2006
This thesis presents the results of numerical simulations on planets embedded in a protoplanetary disk with the hydrodynamics code NIRVANA. We treat the disk as a viscous fluid satisfying the Navier-Stokes equations and integrate these using a finite difference scheme. We present three sets of calculations.
openaire   +1 more source

On the Importance of Wave–Planet Interactions for the Migration of Two Super-Earths Embedded in a Protoplanetary Disk

Astrophysical Journal, 2021
Zijia Cui, Ewa Szuszkiewicz, John C B Papaloizou   +2 more
exaly  

The SPHERE view of the planet-forming disk around HD 100546

Astronomy and Astrophysics, 2016
Christophe Pinte, Silvano Desidera, Arthur Vigan   +2 more
exaly  

Protoplanetary disk lifetimes vs. stellar mass and possible implications for giant planet populations

Astronomy and Astrophysics, 2015
Hervé Bouy, Bruno Merin, Alvaro Ribas   +2 more
exaly  

Decoupling of a giant planet from its disk in an inclined binary system

Astronomy and Astrophysics, 2015
Francesco Marzari, Giovanni Picogna
exaly  

The Criterion for Chaos in Three-Planet Systems and Warped Planet-Disk Interactions

2023
openaire   +1 more source