GJ 273: on the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec

@article{Pozuelos2020GJ2O,
  title={GJ 273: on the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec},
  author={Francisco J. Pozuelos and Juan Carlos Su'arez and Gonzalo C. de El{\'i}a and Z. M. Berdi{\~n}as and Andrea Bonfanti and A. Dugaro and Micha{\"e}l Gillon and Emmanuel Jehin and Maximilian N. G{\"u}nther and Val{\'e}rie Van Grootel and L. J. Garcia and Antoine Thuillier and Laetitia Delrez and Josep Ruiz Rodon},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2020}
}
Planets orbiting low-mass stars such as M dwarfs are now considered a cornerstone in the search for life-harbouring planets. GJ273 is a planetary system orbiting an M dwarf only 3.75 pc away, composed of two confirmed planets, GJ273b and GJ273c, and two promising candidates, GJ273d and GJ273e. Planet GJ273b resides in the habitable zone. Currently, due to a lack of observed planetary transits, only the minimum masses of the planets are known.Despite being an interesting system, the GJ273… 
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