A dynamical investigation of the extrasolar planetary system WASP-3 with special emphasis on transit time variations. Presented at the 8. Alexanxder von Humboldt Colloquium on Celestial Mechanics (March 2011)
18. Stability Diagram:changing test particle mass no big difference between 1, 7 and 15 Earthmasses M=1 MEarth M=7 MEarth M=15 MEarth
19. Constraints? Dynamical constraints on the eccentricity and mass of WASP-3b better constraints on WASP-3c -> more observations -> analysis of resonances WASP-3c lies inside the stable region -> but very close to the chaotic region