Stability constraints in modeling of multi-planet extrasolar systems

Details Stability constraints in modeling of multi-planet extrasolar systems Stability constraints in modeling of multi-planet extrasolar systems

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..249..447g&link_type=abstract

Exoplanets: Detection, Formation and Dynamics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 249, p

Astronomy and Astrophysics

Astronomy

8

Radial Velocity Technique, N-Body Problem, Stars: Hd 155358, Stars: Τ1 Gruis

Scientific paper

We present an analysis of high precision radial velocity (RV) observations of stars hosting multi-planet systems with Jovian companions. We use dynamical stability constraints and quasi-global methods of optimization. As an illustration, we present new results derived for the RV data of the Sun-like dwarfs HD 155358 and τ1 Gruis.

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