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The GAPS programme at TNG

The present-day architecture of planetary systems contains information about their formation and migration histories. The origin of hot Jupiters (HJs; P ≲ 10 d, Rp > 8 R⊕) has long been a matter of debate. While most of them are found to be ‘lonely’, there is a rare population of HJs hosting small i...

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Autors principals: Mantovan G., Nascimbeni V., Desidera S., Malavolta L., Lissauer J. J., Leonardi P., Azevedo Silva T., Guerra C., Polychroni D., Borsato L., Baratella M., Biazzo K., Nardiello D., Collins K. A., Damasso M., De Leon J., Everett M. E., Gandolfi D., Giacalone S., Naponiello L., Piotto G., Scandariato G., Stassun K., Yee S. W., Affer L., Amadori F., Bignamini A., Colombo S., D’Arpa M., Dressing C. D., Fukui A., Ghedina A., Higuera J., Ikuta K., Kawauchi, Korth J., Lorenzi V., Mancini L., Mori M., Murgas F., Narita N., Palle E., Parviainen H., Ruggieri A., Savel A., Schwarz R. P., Shporer A., Srdoc G., Stockdale, Watanabe D., Zambelli R., Zingales T.
Format: Artigo
Idioma:Inglês
Publicat: EDP Sciences 2026-09-01
Col·lecció:Astronomy & Astrophysics
Matèries:
planets and satellites: fundamental parameters
planets and satellites: gaseous planets
stars: fundamental parameters
Accés en línia:https://www.aanda.org/articles/aa/full_html/2026/09/aa60961-26/aa60961-26.html
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