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A cool runaway greenhouse without surface magma ocean. <i>Nature (Lond.) 620(7973)</i>: 287-291. <a href=\"https://dx.doi.org/10.1038/s41586-023-06258-3\" target=\"_blank\">https://dx.doi.org/10.1038/s41586-023-06258-3</a>","AutID":467829,"MonDate":null,"AnaDate":2023,"PeerRev":1,"outputType":"1_A1","OpenAcc":0},{"BRefID":345776,"RR":"<b>Turbet, M.; Bolmont, E.; Chaverot, G.; Ehrenreich, D.; Leconte, J.; Marcq, E.</b> (2021). Day–night cloud asymmetry prevents early oceans on Venus but not on Earth. <i>Nature (Lond.) 598(7880)</i>: 276-280. <a href=\"https://dx.doi.org/10.1038/s41586-021-03873-w\" target=\"_blank\">https://dx.doi.org/10.1038/s41586-021-03873-w</a>","AutID":467829,"MonDate":null,"AnaDate":2021,"PeerRev":1,"outputType":"1_A1","OpenAcc":0},{"BRefID":285328,"RR":"<b>Bolmont, E.; Selsis, F.; Owen, J.E.; Ribas, I.; Raymond, S.N.; Leconte, J.; Gillon, M.</b> (2017). Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1. <i>Monthly Notices of the Royal Astronomical Society 464(3)</i>: 3728-3741. <a href=\"https://dx.doi.org/10.1093/mnras/stw2578\" target=\"_blank\">https://dx.doi.org/10.1093/mnras/stw2578</a>","AutID":272403,"MonDate":null,"AnaDate":2017,"PeerRev":1,"outputType":"1_A1","OpenAcc":0},{"BRefID":295593,"RR":"<b>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.</b> (2017). Temporal evolution of the high-energy irradiation and water content of TRAPPIST-1 exoplanets. <i>Astronomical Journal 154(3)</i>: 1-17. <a href=\"https://dx.doi.org/10.3847/1538-3881/aa859c\" target=\"_blank\">https://dx.doi.org/10.3847/1538-3881/aa859c</a>","AutID":326185,"MonDate":null,"AnaDate":2017,"PeerRev":1,"outputType":"1_A1","OpenAcc":1},{"BRefID":285554,"RR":"<b>Bolmont, E.; Libert, A.-S.; Leconte, J.; Selsis, F.</b> (2016). Habitability of planets on eccentric orbits: limits of the mean flux approximation. <i>Astron. Astrophys. 591</i>: 17 pp. <a href=\"https://dx.doi.org/10.1051/0004-6361/201628073\" target=\"_blank\">https://dx.doi.org/10.1051/0004-6361/201628073</a>","AutID":272403,"MonDate":null,"AnaDate":2016,"PeerRev":1,"outputType":"1_A1","OpenAcc":0},{"BRefID":285420,"RR":"<b>Bolmont, E.; Mathis, S.</b> (2016). Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets. <i>Celestial Mechanics & Dynamical Astronomy 126(1)</i>: 275-296. <a href=\"https://dx.doi.org/10.1007/s10569-016-9690-3\" target=\"_blank\">https://dx.doi.org/10.1007/s10569-016-9690-3</a>","AutID":272403,"MonDate":null,"AnaDate":2016,"PeerRev":1,"outputType":"1_A1","OpenAcc":0},{"BRefID":338202,"RR":"<b>Turbet, M.; Leconte, J.; Selsis, F.; Bolmont, E.; Forget, F.; Ribas, I.; Raymond, S.N.; Anglada-Escudé, G.</b> (2016). The habitability of Proxima Centauri b. II. Possible climates and observability. <i>Astron. Astrophys. 596</i>: A112. <a href=\"https://hdl.handle.net/10.1051/0004-6361/201629577\" target=\"_blank\">https://hdl.handle.net/10.1051/0004-6361/201629577</a>","AutID":272403,"MonDate":null,"AnaDate":2016,"PeerRev":1,"outputType":"1_A1","OpenAcc":1}]},"urls":null,"spcols":null,"thesterms":null,"taxterms":null,"pub":1,"newses":{"SesID":85279,"LoginName":"VLIZ2000\\zohrab","LoginID":435,"DD":"2017-06-14"},"updses":{"SesID":85279,"LoginName":"VLIZ2000\\zohrab","LoginID":435,"DD":"2017-06-14"},"urlmaps":[],"resmessage":"no id specified","complete":1}