Articles citing this article

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Cited article:

Planet population synthesis: the role of stellar encounters

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Monthly Notices of the Royal Astronomical Society 512 (1) 861 (2022)
https://doi.org/10.1093/mnras/stac569

Close stellar encounters kicking planets out of habitable zone in various stellar environments

Behzad Bojnordi Arbab and Sohrab Rahvar
International Journal of Modern Physics D 30 (09) 2150063 (2021)
https://doi.org/10.1142/S0218271821500632

Dynamics of passing-stars-perturbed binary star systems

D Bancelin, T Nordlander, E Pilat-Lohinger and B Loibnegger
Monthly Notices of the Royal Astronomical Society 486 (4) 4773 (2019)
https://doi.org/10.1093/mnras/stz1173

Tails and bridges in the parabolic restricted three-body problem

Esther Barrabés, Josep M. Cors, Laura Garcia-Taberner and Mercè Ollé
Monthly Notices of the Royal Astronomical Society 472 (3) 2554 (2017)
https://doi.org/10.1093/mnras/stx1990

Generation of inclined protoplanetary discs and misaligned planets through mass accretion – I. Coplanar secondary discs

M. Xiang-Gruess and P. Kroupa
Monthly Notices of the Royal Astronomical Society 471 (2) 2334 (2017)
https://doi.org/10.1093/mnras/stx1651

Generation of highly inclined protoplanetary discs through single stellar flybys

M. Xiang-Gruess
Monthly Notices of the Royal Astronomical Society 455 (3) 3086 (2016)
https://doi.org/10.1093/mnras/stv2514

Dynamics of the parabolic restricted three-body problem

Esther Barrabés, Josep M. Cors and Mercè Ollé
Communications in Nonlinear Science and Numerical Simulation 29 (1-3) 400 (2015)
https://doi.org/10.1016/j.cnsns.2015.05.025

Effects of stellar flybys on planetary systems: 3D modeling of the circumstellar disk’s damping effects

G. Picogna and F. Marzari
Astronomy & Astrophysics 564 A28 (2014)
https://doi.org/10.1051/0004-6361/201322816

THE HIGHLY DYNAMIC BEHAVIOR OF THE INNERMOST DUST AND GAS IN THE TRANSITION DISK VARIABLE LRLL 31

K. M. Flaherty, J. Muzerolle, G. Rieke, et al.
The Astrophysical Journal 732 (2) 83 (2011)
https://doi.org/10.1088/0004-637X/732/2/83