The GAPS Programme at TNG: XXXVII. A precise density measurement of the young ultra-short period planet TOI-1807 b

Context. Great strides have been made in recent years in the understanding of the mechanisms involved in the formation and evolution of planetary systems. Despite this, many observational findings have not yet been corroborated by astrophysical explanations. A fine contribution to the study of plane...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2022-08, Vol.664, p.A163
Hauptverfasser: Nardiello, D., Malavolta, L., Desidera, S., Baratella, M., D’Orazi, V., Messina, S., Biazzo, K., Benatti, S., Damasso, M., Rajpaul, V. M., Bonomo, A. S., Capuzzo Dolcetta, R., Mallonn, M., Cale, B., Plavchan, P., El Mufti, M., Bignamini, A., Borsa, F., Carleo, I., Claudi, R., Covino, E., Lanza, A. F., Maldonado, J., Mancini, L., Micela, G., Molinari, E., Pinamonti, M., Piotto, G., Poretti, E., Scandariato, G., Sozzetti, A., Andreuzzi, G., Boschin, W., Cosentino, R., Fiorenzano, A. F. M., Harutyunyan, A., Knapic, C., Pedani, M., Affer, L., Maggio, A., Rainer, M.
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Sprache:eng
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Zusammenfassung:Context. Great strides have been made in recent years in the understanding of the mechanisms involved in the formation and evolution of planetary systems. Despite this, many observational findings have not yet been corroborated by astrophysical explanations. A fine contribution to the study of planetary formation processes comes from the study of young, low-mass planets, with short orbital periods (
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202243743