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Cited article:

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Habitable Planet Formation around Low-mass Stars: Rapid Accretion, Rapid Debris Removal, and the Essential Contribution of External Giants

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

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Sublimation of icy planetesimals and the delivery of water to the habitable zone around solar type stars

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

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