41 citations · 80 across the 2 of their papers we have counts for
8 papers
Pushing planets into an inner cavity by a resonant chain
S. Ataiee, W. Kley
Context. The orbital distribution of exoplanets indicates an accumulation of super-Earth sized planets close to their host stars in compact systems. When an inward disc-driven migr…
The role of disc torques in forming resonant planetary systems
S. Ataiee, W. Kley
The most accurate method for modelling planetary migration and hence the formation of resonant systems is using hydrodynamical simulations. Usually, the force (torque) acting on a…
The impact of planet wakes on the location and shape of the water iceline in a protoplanetary disk
Alexandros Ziampras, Sareh Ataiee, Wilhelm Kley +2
Context: Planets in accretion disks can excite spiral shocks, and---if massive enough---open gaps in their vicinity. Both of these effects can influence the overall disk thermal st…
1:1 orbital resonance of circumbinary planets
Anna B. T. Penzlin, Sareh Ataiee, Wilhelm Kley
The recent detection of the third planet in Kepler-47 has shown that binary stars can host several planets in circumbinary orbits. To understand the evolution of such systems we ha…
Stability of the co-orbital resonance under dissipation: Application to its evolution in protoplanetary discs
Adrien Leleu, Gavin Coleman, Sareh Ataiee
Despite the existence of co-orbital bodies in the solar system, and the prediction of the formation of co-orbital planets by planetary system formation models, no co-orbital exopla…
The formation of Jupiter by hybrid pebble-planetesimal accretion
Yann Alibert, Julia Venturini, Ravit Helled +8
The standard model for giant planet formation is based on the accretion of solids by a growing planetary embryo, followed by rapid gas accretion once the planet exceeds a so-called…