Long-term monitoring of WASP-19 b: Signs of apsidal precession and molecular signatures

Context. With over 6000 exoplanets discovered to date, approximately 12 % are classified as hot-Jupiters. Due to their large sizes and short orbital periods (P < 10 day), they are easier to detect and provide crucial insights into planetary formation, atmospheric properties, and orbital dynamics. Am...

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Autori principali:	Rajkumar A. R., Bayo A., Peng P., Tregloan-Reed J., Southworth J., Hinse Tobias C., Alegre L. G., Amadio F., Andersen M., Bach-Møller N., Basilicata M., Bonavita M., Bozza V., Burgdorf M. J., Cannon R. E., Columba G., Dominik M., Donaldson A., Figuera Jaimes R., Fynbo J., Hundertmark M., Jørgensen U. G., Khalouei E., Korhonen H., Longa-Peña P., Mancini L., Rabus M., Rahvar S., Rendell-Bhatti H., Rota P., Rozek A., Sajadian S., Skottfelt J., Snodgrass C.
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	EDP Sciences 2026-04-01
Serie:	Astronomy & Astrophysics
Soggetti:	techniques: photometric techniques: spectroscopic planets and satellites: atmospheres planets and satellites: dynamical evolution and stability planet-star interactions
Accesso online:	https://www.aanda.org/articles/aa/full_html/2026/04/aa56822-25/aa56822-25.html
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