Stability constraints in modeling of multi-planet extrasolar systems

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dc.creatorGozdziewski, K.
dc.creatorMigaszewski, C.
dc.creatorMusielinski, A.
dc.date2008-02-02
dc.date.accessioned2026-07-07T09:18:28Z
dc.date.available2026-07-07T09:18:28Z
dc.descriptionWe 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 $τ^1$ Gruis.
dc.description13 pages, to appear in the Proceedings of IAU Symposium 249, Suzhou (China) "Exoplanets: Detection, Formation and Dynamics", eds. Y.-S. Sun, S. Ferraz-Mello, J.-L. Zhou. Please download pdf for acceptable quality of figures (see also http://www.astri.uni.torun.pl/~chris/iau249.pdf)
dc.identifierhttps://arxiv.org/abs/0802.0254
dc.identifierhttp://arxiv.org/abs/0802.0254
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/154033
dc.subjectAstrophysics
dc.titleStability constraints in modeling of multi-planet extrasolar systems
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