• Aucun résultat trouvé

Dynamics of the giant planets of the solar system in the gaseous proto-planetary disk and relationship to the current orbital architecture

N/A
N/A
Protected

Academic year: 2021

Partager "Dynamics of the giant planets of the solar system in the gaseous proto-planetary disk and relationship to the current orbital architecture"

Copied!
39
0
0

Texte intégral

Loading

Références

Documents relatifs

Im Rahmen eines Krampf- anfalls kann es infolge der raschen Zu- nahme osmotisch-aktiver Teilchen (z. durch den Abbau von Glykogen in kleine- re Moleküle wie Laktat) im

Les pharmaciens sont certainement les professionnels les plus sensibilisés au besoin de procéder à ces ajustements et ont été les apôtres de l’estimation de la fonction rénale

In this case, the difference of electric potential induced by the planet’s relative motion with respect to the magnetic field of its host star drives an electrical current out of

The number of transitions one needs to forbid for a graph to lose its Hamiltonicity gives a measure of its robustness: if the smallest set of forbidden transitions that makes a

We observed functional variations in her Toll like 5 receptor (TLR 5) gene and two coagulation variations (Tissue Factor (TF) 603 and Plasminogen-Activator-Inhibitor-1 (PAI-1)

Integrative analysis of the cancer genome atlas and cancer cell lines encyclopedia large-scale genomic databases: MUC4/MUC16/MUC20 signature is associated with poor survival in

Comparing the distributions of the durations of Ganymede–Jupiter and Io–Jupiter emission events also suggests that while the latter results from quasi-permanent Alfvén wave

In order, to understand the integrated effect of the riblets on the structure of a viscous boundary layer, it is important to first systematically unravel how the laminar boundary