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Des super-Terres accueillantes = Welcoming super-EarthsSASSELOV, Dimitar; VALENCIA, Dian.Pour la science (Imprimé). 2010, Num 396, pp 50-57, issn 0153-4092, 8 p.Article
Alien Planets Hit the Commodities Market : Insights of the DecadeBHATTACHARJEE, Yudhijit.Science (Washington, D.C.). 2010, Vol 330, Num 6011, issn 0036-8075, p. 1620Article
A Giant Planet Around a Metal-Poor Star of Extragalactic OriginSETIAWAN, Johny; KLEMENT, Rainer J; HENNING, Thomas et al.Science (Washington, D.C.). 2010, Vol 330, Num 6011, pp 1642-1644, issn 0036-8075, 3 p.Article
Les planètes (les nôtres et les autres)Encrenaz, Thérèse; Lequeux, James.Une Introduction à. 2010, issn 2108-5978, isbn 978-2-7598-0444-3, 1Vol, 187 p., isbn 978-2-7598-0444-3Book
Trop grosse pour être une planète = Too big for a planetLE MEUR, Hélène.La Recherche (Imprimé). 2009, Num 426, pp 47-49, issn 0029-5671, 3 p.Article
The presence of methane in the atmosphere of an extrasolar planetSWAIN, Mark R; VASISHT, Gautam; TINETTI, Giovanna et al.Nature (London). 2008, Vol 452, Num 7185, pp 329-331, issn 0028-0836, 3 p.Article
Strong water absorption in the dayside emission spectrum of the planet HD 189733bGRILLMAIR, Carl J; BURROWS, Adam; CHARBONNEAU, David et al.Nature (London). 2008, Vol 456, Num 7223, pp 767-769, issn 0028-0836, 3 p.Article
Energetic neutral atoms as the explanation for the high-velocity hydrogen around HD 209458bHOLMSTRÖM, M; EKENBÄCK, A; SELSIS, F et al.Nature (London). 2008, Vol 451, Num 7181, pp 970-972, issn 0028-0836, 3 p.Article
The hottest planetHARRINGTON, Joseph; LUSZCZ, Statia; SEAGER, Sara et al.Nature (London). 2007, Vol 447, Num 7145, pp 691-693, issn 0028-0836, 3 p.Article
Planet-planet scattering in the upsilon Andromedae systemFORD, Eric B; LYSTAD, Verene; RASIO, Frederic A et al.Nature (London). 2005, Vol 434, Num 7035, pp 873-876, issn 0028-0836, 4 p.Article
Cooler and bigger than previously thought? Planetary host stellar parameters from the infrared flux methodRAMIREZ, Ivan; MELENDEZ, Jorge.The Astrophysical journal. 2004, Vol 609, Num 1, pp 417-422, issn 0004-637X, 6 p., 1Article
Multiple companions to HD 154857 and HD 160691MCCARTHY, Chris; BUTLER, R. Paul; TINNEY, C. G et al.The Astrophysical journal. 2004, Vol 617, Num 1, pp 575-579, issn 0004-637X, 5 p., 1Article
Toward a deterministic model of planetary formation. II. The formation and retention of gas giant planets around stars with a range of metallicitiesIDA, Shigeru; LIN, D. N. C.The Astrophysical journal. 2004, Vol 616, Num 1, pp 567-572, issn 0004-637X, 6 p., 1Article
An abundance of small exoplanets around stars with a wide range of metallicitiesBUCHHAVE, Lars A; LATHAM, David W; BRYSON, Stephen T et al.Nature (London). 2012, Vol 486, Num 7403, pp 375-377, issn 0028-0836, 3 p.Article
One or more bound planets per Milky Way star from microlensing observationsCASSAN, A; KUBAS, D; UDALSKI, A et al.Nature (London). 2012, Vol 481, Num 7380, pp 167-169, issn 0028-0836, 3 p.Article
The signature of orbital motion from the dayside of the planet τ Boötis bBROGI, Matteo; SNELLEN, Ignas A. G; DE KOK, Remco J et al.Nature (London). 2012, Vol 486, Num 7404, pp 502-504, issn 0028-0836, 3 p.Article
Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing VariationsHOLMAN, Matthew J; FABRYCKY, Daniel C; BATALHA, Natalie M et al.Science (Washington, D.C.). 2010, Vol 329, Num 6000, pp 51-54, issn 0036-8075, 4 p.Article
The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and JupitersHOWARD, Andrew W; MARCY, Geoffrey W; ASHER JOHNSON, John et al.Science (Washington, D.C.). 2010, Vol 330, Num 6004, pp 653-655, issn 0036-8075, 3 p.Article
New worlds on the horizon : Earth-sized planets close to other starsGAIDOS, Eric; HAGHIGHIPOUR, Nader; AGOL, Eric et al.Science (Washington, D.C.). 2007, Vol 318, Num 5848, pp 210-213, issn 0036-8075, 4 p.Article
Extrasolar planets : Constraints for planet formation modelsSANTOS, Nuno C; BENZ, Willy; MAYOR, Michel et al.Science (Washington, D.C.). 2005, Vol 310, Num 5746, pp 251-255, issn 0036-8075, 5 p.Article
Predicting planets in known extrasolar planetary systems. II. Testing for saturn mass planetsRAYMOND, Sean N; BARNES, Rory.The Astrophysical journal. 2005, Vol 619, Num 1, pp 549-557, issn 0004-637X, 9 p., 1Article
Quand les planètes perdent leur atmosphère = When planets lose their atmosphereLECAVELIER DES ETANGS, Alain.Pour la science. 2005, Num 334, pp 54-60, issn 0153-4092, 7 p.Article
Effects of helium phase separation on the evolution of extrasolar giant planetsFORTNEY, Jonathan J; HUBBARD, W. B.The Astrophysical journal. 2004, Vol 608, Num 2, pp 1039-1049, issn 0004-637X, 11 p., 1Article
A minimum-mass extrasolar nebulaKUCHNER, Marc J.The Astrophysical journal. 2004, Vol 612, Num 2, pp 1147-1151, issn 0004-637X, 5 p., 1Article
Apsidal corotation in mean motion resonance: the 55 Cancri system as an exampleZHOU, Li-Yong; LEHTO, Harry J; SUN, Yi-Sui et al.Monthly Notices of the Royal Astronomical Society. 2004, Vol 350, Num 4, pp 1495-1502, issn 0035-8711, 8 p.Article