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Autor:
Adelbert, Stefan, Penzlin, Anna B. T., Schäfer, Christoph M., Kley, Wilhelm, Quarles, Billy, Sfair, Rafael
Publikováno v:
A&A 680, A29 (2023)
In previous hydrodynamical simulations, we found a mechanism for nearly circular binary stars, like Kepler-413, to trap two planets in a stable 1:1 resonance. Therefore, the stability of coorbital configurations becomes a relevant question for planet
Externí odkaz:
http://arxiv.org/abs/2310.07575
