On the interaction between embedded planets and the corotation region of protoplanetary discs [PDF]
PhDDisc material in the corotation region librates with respect to low-mass planets on horseshoe trajectories. The exchange of angular momentum associated with this libration gives rise to the non-linear corotation torque (the horseshoe drag).
Fendyke, Stephen
core +4 more sources
TOI-1859b: A 64 Day Warm Jupiter on an Eccentric and Misaligned Orbit
Warm Jupiters are close-in giant planets with relatively large planet–star separations (i.e., 10 < a / R _⋆ < 100). Given their weak tidal interactions with their host stars, measurements of stellar obliquity may be used to probe the initial obliquity ...
Jiayin Dong +33 more
doaj +1 more source
Disk evolution, element abundances and cloud properties of young gas giant planets [PDF]
ChHc and PBR highlights financial support of the European Community under the FP7 program by an ERC starting grant. PW, IK, and WFT acknowledge funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement No.
Kamp, I. +19 more
core +2 more sources
Gap formation in a self-gravitating disk and the associated migration of the embedded giant planet [PDF]
We present the results of our recent study on the interactions between a giant planet and a self-gravitating gas disk. We investigate how the disk's self-gravity affects the gap formation process and the migration of the giant planet.
Zhang, Hui +3 more
core +1 more source
Constraining the gas distribution in the PDS 70 disk as a method to assess the effect of planet-disk interactions [PDF]
Embedded planets are potentially the cause of substructures like gaps and cavities observed in several protoplanetary disks. Thus, the substructures observed in the continuum and in line emission encode information about the presence of planets in the ...
Law, C. +25 more
core +1 more source
Star-planet interactions [PDF]
When planets are formed from the protoplanetary disk and after the disk has dissipated, the evolution of their orbits is governed by tidal interactions, friction, and gravitational drag, and also by changes in the mass of the star and planet.
Lionel Haemmerlé +15 more
core +3 more sources
Star-planet interactions [PDF]
Context. Tidal interactions and planetary evaporation processes impact the evolution of close-in star–planet systems. Aims. We study the impact of stellar rotation on these processes. Methods.
Vincent Bourrier +17 more
core +3 more sources
Characterizing circumstellar disk around young stars [PDF]
The circumstellar disks play a fundamental role in star and planet formation process. Studies on circumstellar disks are generally carried on following two viable approaches: "statistical" studies, where a large samples of sources are measured to ...
Schisano, Eugenio
core +1 more source
Gas phase ion species released during grain collisions: Implications for protoplanetary disks
Grain charging and gas ionization are important processes in protoplanetary disks. Both occur in mutual collisions between grains, as charge is exchanged between grain surfaces but also released into the surrounding gas as ions.
Hock P., Wurm G.
doaj +1 more source
Dynamics of the TWA 7 planetary system and possibility of an additional planet
Context. The debris disk surrounding the young star TWA 7 exhibits morphological features that tightly constrain its planetary architecture. JWST/MIRI observations have recently revealed a directly imaged outer planet orbiting at a large separation.
Lacquement A. +3 more
doaj +1 more source

