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Cited article:

Rocky planet formation in compact disks around M dwarfs

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Dynamical Packing in the Habitable Zone: The Case of Beta CVn

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The Astronomical Journal 160 (2) 81 (2020)
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GJ 273: on the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec

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Water worlds in N-body simulations with fragmentation in systems without gaseous giants

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Physical properties of terrestrial planets and water delivery in the habitable zone using N-body simulations with fragmentation

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Astronomy & Astrophysics 632 A14 (2019)
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Planetary formation and water delivery in the habitable zone around solar-type stars in different dynamical environments

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Astronomy & Astrophysics 609 A76 (2018)
https://doi.org/10.1051/0004-6361/201730848

Formation of Solar system analogues – II. Post-gas-phase growthand water accretion in extended discs via N-body simulations

M P Ronco and G C de Elía
Monthly Notices of the Royal Astronomical Society 479 (4) 5362 (2018)
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Effects of an eccentric inner Jupiter on the dynamical evolution of icy body reservoirs in a planetary scattering scenario

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Formation of solar system analogues – I. Looking for initial conditions through a population synthesis analysis

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Migrating Jupiter up to the habitable zone: Earth-like planet formation and water delivery

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Astronomy & Astrophysics 607 A63 (2017)
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Detectable close-in planets around white dwarfs through late unpacking

Dimitri Veras and Boris T. Gänsicke
Monthly Notices of the Royal Astronomical Society 447 (2) 1049 (2015)
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Terrestrial planet formation in low-mass disks: dependence with initial conditions

M. P. Ronco, G. C. de Elía and O. M. Guilera
Proceedings of the International Astronomical Union 9 (S310) 218 (2014)
https://doi.org/10.1017/S174392131400831X