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New Jupiter and Saturn formation models meet observations

, , , and . ASTROPHYSICAL JOURNAL, 626 (1): L57--L60 (June 2005)

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The D/H Ratio in Methane in Titan: Origin and History, , and . Icarus, 159 (1): 156--165 (2002)The photophoretic sweeping of dust in transient protoplanetary disks, , , , , and . \aap, (February 2007)Liquid water on Enceladus from observations of ammonia and $^40$Ar in the plume, , , , , , , , , and 6 other author(s). Nature, 460 (7254): 487--490 (Jul 23, 2009)Modeling the Jovian subnebulaI. Thermodynamic conditions and migration of proto-satellites, , and . ASTRONOMY & ASTROPHYSICS, 439 (3): 1205--1213 (September 2005)New Jupiter and Saturn formation models meet observations, , , and . ASTROPHYSICAL JOURNAL, 626 (1): L57--L60 (June 2005)Formation of giant planetsAn attempt in matching observational constraints, , , and . SPACE SCIENCE REVIEWS, 116 (1-2): 77--95 (2005)On the volatile enrichments and composition of Jupiter, , and . ASTROPHYSICAL JOURNAL, 622 (2): L145--L148 (April 2005)Sequestration of Ethane in the Cryovolcanic Subsurface of Titan, , , , , , , , , and 1 other author(s). The Astrophysical Journal, 677 (1): L67--L70 (2008)Experiments in the NH$_3$-H$_2$O system in the 0,1 GPa pressure range - implications for the deep liquid layer of large icy satellites, , , and . Geophysical Research Letters, 29 (24): 2192 (2002)On the composition of ices incorporated in Ceres, and . MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 358 (1): 188--192 (March 2005)