The TROY project. II. Multi-technique constraints on exotrojans in nine planetary systems
Context. Co-orbital bodies are the byproduct of planet formation and evolution, as we know from the solar system. Although planet-size co-orbitals do not exists in our planetary system, dynamical studies show that they can remain stable for long periods of time in the gravitational well of massive planets. Should they exist, their detection is
Lillo-Box, J. et al.
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2018