Host star properties of hot, warm and cold Jupiters in the solar neighborhood from Gaia DR3: clues to formation pathways

Giant planets exhibit diverse orbital properties, hinting at their distinct formation and dynamic histories. In this paper, using \textit{Gaia} DR3, we investigate if and how the orbital properties of Jupiters are linked to their host star properties, particularly their metallicity and age. We obtain metallicities for main sequence stars of... Show more