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Formation of solar system analogues - I. Looking for initial conditions through a population synthesis analysis
(Oxford University Press, 2017-11)
Population synthesis models of planetary systems developed during the last ~15 yr could reproduce several of the observables of the exoplanet population, and also allowed us to constrain planetary formation models. We ...
Dynamic portrait of the planetary 2/1 mean-motion resonance - II. Systems with a more massive inner planet
(WILEY-BLACKWELL PUBLISHING, INC, 2008)
This paper presents the second part in our study of the global structure of the planar phase space of the planetary three-body problem, when both planets lie in the vicinity of a 2/1 mean-motion resonance. While Paper I ...
OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion?
(2009)
We combine all available information to constrain the nature of OGLE-2005-BLG-071Lb, the second planet discovered by microlensing and the first in a high-magnification event. These include photometric and astrometric ...
GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec
(EDP Sciences, 2020-09)
Context. Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for planets with thepotential to harbour life. GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, ...