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Orbital structure of planetary systems formed by giant impacts: stellar mass dependence

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Monthly Notices of the Royal Astronomical Society 519 (2) 2838 (2022)
https://doi.org/10.1093/mnras/stac3756

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

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Role of gaseous giants in the dynamical evolution of terrestrial planets and water delivery in the habitable zone

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Monthly Notices of the Royal Astronomical Society 481 (1) 1281 (2018)
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Planetary formation and water delivery in the habitable zone around solar-type stars in different dynamical environments

P. S. Zain, G. C. de Elía, M. P. Ronco and O. M. Guilera
Astronomy & Astrophysics 609 A76 (2018)
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Formation of Solar system analogues – II. Post-gas-phase growthand water accretion in extended discs via N-body simulations

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Monthly Notices of the Royal Astronomical Society 479 (4) 5362 (2018)
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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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Characterising face-on accretion onto and the subsequent contraction of protoplanetary discs

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FORMATION, TIDAL EVOLUTION, AND HABITABILITY OF THE KEPLER-186 SYSTEM

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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