Coorbital planets: Radial velocity detection

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Coorbital planets: Radial velocity detection

Post by Lazarus on 4th December 2011, 12:06 pm

Origin and Detectability of coorbital planets from radial velocity data

Various results come out of this: a 1:1 resonance can be confused with other configurations, but the other incorrect configurations are often unstable. However the approach of fitting planets sequentially can result in stable incorrect configurations.
dG star
dG star

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