Abstract
Dynamical studies of new exoplanet systems are a critical component of the discovery and characterisation process. Such studies can provide firmer constraints on the parameters of the newly discovered planets, and may even reveal that the proposed planets do not stand up to dynamical scrutiny. Here, we demonstrate how dynamical studies can assist the characterisation of such systems through two examples: QS Virginis and HD 73526. Copyright © 2013, International Astronomical Union.
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Horner, J., Wittenmyer, R. A., Tinney, C., Hinse, T. C., & Marshall, J. P. (2013). Dynamical constraints on exoplanets. In Proceedings of the International Astronomical Union (Vol. 8, pp. 293–294). Cambridge University Press. https://doi.org/10.1017/S174392131300865X
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