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A sample of 46 stars, host of exoplanets, is used to search for a connectionbetween their formation process and the formation of the planets rotatingaround them. Separating our sample in two, stars hosting high-mass exoplanets(HMEs) and low-mass exoplanets (LMEs), we found the former to be more massiveand to rotate faster than the latter. We also found the HMEs to have higherorbital angular momentum than the LMEs and to have lost more angular momentumthrough migration. These results are consistent with the view that the moremassive the star and higher its rotation, the more massive was itsprotoplanetarys disk and rotation, and the more efficient the extraction ofangular momentum from the planets.

Connecting the formation of stars and planets. II: coupling the angular momentum of stars with the angular momentum of planets