| Vorig instituut |
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Université de Namur; Département de mathématique; Centre Namurois des Systèmes Complexes - naXys (naXys), meer
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| Publicaties (7) |
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| A1 publicaties (7) [show] |
- Selsis, F.; Leconte, J.; Turbet, M.; Chaverot, G.; Bolmont, E. (2023). A cool runaway greenhouse without surface magma ocean. Nature (Lond.) 620(7973): 287-291. https://dx.doi.org/10.1038/s41586-023-06258-3, meer
- Turbet, M.; Bolmont, E.; Chaverot, G.; Ehrenreich, D.; Leconte, J.; Marcq, E. (2021). Day–night cloud asymmetry prevents early oceans on Venus but not on Earth. Nature (Lond.) 598(7880): 276-280. https://dx.doi.org/10.1038/s41586-021-03873-w, meer
- Bolmont, E.; Selsis, F.; Owen, J.E.; Ribas, I.; Raymond, S.N.; Leconte, J.; Gillon, M. (2017). Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1. Monthly Notices of the Royal Astronomical Society 464(3): 3728-3741. https://dx.doi.org/10.1093/mnras/stw2578, meer
 Bourrier, V.; de Wit, J.; Bolmont, E.; Stamenkovic, V.; Wheatley, P.J.; Burgasser, A.J.; Delrez, L.; Demory, B.O.; Ehrenreich, D.; Gillon, M.; Jehin, E.; Leconte, J.; Lederer, S.M.; Lewis, N.; Triaud, A.H.M.J.; Van Grootel, V. (2017). Temporal evolution of the high-energy irradiation and water content of TRAPPIST-1 exoplanets. Astronomical Journal 154(3): 1-17. https://dx.doi.org/10.3847/1538-3881/aa859c, meer- Bolmont, E.; Libert, A.-S.; Leconte, J.; Selsis, F. (2016). Habitability of planets on eccentric orbits: limits of the mean flux approximation. Astron. Astrophys. 591: 17 pp. https://dx.doi.org/10.1051/0004-6361/201628073, meer
- Bolmont, E.; Mathis, S. (2016). Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets. Celestial Mechanics & Dynamical Astronomy 126(1): 275-296. https://dx.doi.org/10.1007/s10569-016-9690-3, meer
- Turbet, M.; Leconte, J.; Selsis, F.; Bolmont, E.; Forget, F.; Ribas, I.; Raymond, S.N.; Anglada-Escudé, G. (2016). The habitability of Proxima Centauri b. II. Possible climates and observability. Astron. Astrophys. 596: A112. https://hdl.handle.net/10.1051/0004-6361/201629577, meer
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