Add to ORKGWe investigate the effects of a passing stellar encounter on a planetesimal disk through analytical calculations and numerical simulations, and derive the boundary radius ($a_{\rm planet}$) outside which planet formation is inhibited by disruptive collisions with high relative velocities
We have investigated the final accretion stage of terrestrial planets from Mars-mass protoplanets th...
Monthly Notices of the Royal Astronomical Society, 380, pp. 1119-1126, http://dx.doi.org./10.1111/j....
Observations of extrasolar planets reveal that planets can be found in close binary systems, where t...
Context. The majority of stars in the Galaxy are thought to have formed within stellar clusters, res...
Context. A large fraction of stars, including young T Tauri stars, are observed to be memb...
In this thesis I investigate the formation and dynamics of planets and protoplanetary discs, subject...
Context. Stellar flybys in star clusters are suspected of affecting the orbital architecture of plan...
Stellar flybys in star clusters may perturb the evolution of young planetary systems in terms of dis...
The existence of planets born in environments highly perturbed by a stellar companion represents a m...
Monthly Notices of the Royal Astronomical Society, 388, pp. 1528-1536, http://dx.doi.org./10.1111/j....
The extent to which planetesimal accretion is affected by the perturbing presence of a companion sta...
Aims: We explore planet formation in binary systems around the central star where the protoplanetary...
Context. Most stars form in embedded clusters. Stellar flybys may affect the orbital architecture of...
Context. Most stars form in embedded clusters. Stellar flybys may affect the orbital architecture of...
We numerically explore planet formation around \u3b1 Centauri A by focusing on the crucial planetesi...
We have investigated the final accretion stage of terrestrial planets from Mars-mass protoplanets th...
Monthly Notices of the Royal Astronomical Society, 380, pp. 1119-1126, http://dx.doi.org./10.1111/j....
Observations of extrasolar planets reveal that planets can be found in close binary systems, where t...
Context. The majority of stars in the Galaxy are thought to have formed within stellar clusters, res...
Context. A large fraction of stars, including young T Tauri stars, are observed to be memb...
In this thesis I investigate the formation and dynamics of planets and protoplanetary discs, subject...
Context. Stellar flybys in star clusters are suspected of affecting the orbital architecture of plan...
Stellar flybys in star clusters may perturb the evolution of young planetary systems in terms of dis...
The existence of planets born in environments highly perturbed by a stellar companion represents a m...
Monthly Notices of the Royal Astronomical Society, 388, pp. 1528-1536, http://dx.doi.org./10.1111/j....
The extent to which planetesimal accretion is affected by the perturbing presence of a companion sta...
Aims: We explore planet formation in binary systems around the central star where the protoplanetary...
Context. Most stars form in embedded clusters. Stellar flybys may affect the orbital architecture of...
Context. Most stars form in embedded clusters. Stellar flybys may affect the orbital architecture of...
We numerically explore planet formation around \u3b1 Centauri A by focusing on the crucial planetesi...
We have investigated the final accretion stage of terrestrial planets from Mars-mass protoplanets th...
Monthly Notices of the Royal Astronomical Society, 380, pp. 1119-1126, http://dx.doi.org./10.1111/j....
Observations of extrasolar planets reveal that planets can be found in close binary systems, where t...