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Stability constraints in modeling of multi-planet extrasolar systems
Astrophysics · Submitted 2 Feb 2008
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim As an illustration, we present new results derived for the RV data of the Sun-like dwarfs HD 155358 and $\tau^1$ Gruis.
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The abstract, sentence by sentence
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 $\tau^1$ Gruis.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We present an analysis of high precision radial velocity (RV) observations of stars hosting multi-planet systems with Jovian companions. | contribution 0.89 | 0.92 | 0.04 | asserted 0.96 |
| s1 | We use dynamical stability constraints and quasi-global methods of optimization. | method 1.00 | 0.90 | 0.06 | asserted 0.96 |
| s2 | As an illustration, we present new results derived for the RV data of the Sun-like dwarfs HD 155358 and $\tau^1$ Gruis. | contribution 0.72 | 0.95 | 0.06 | asserted 0.99 |
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The paper
Original abstract
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 $\tau^1$ Gruis.
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2 arXiv papers cite this in 2 sentences
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[ref] and [ref] utilize stability constraints and optimization techniques partly derived from the MEGNO (Mean Exponential Growth Factor for Nearby Orbits) method [ref] .
Secular Orbital Dynamics of Hierarchical Two Planet Systems · Introduction · 0.80
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