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Context. The transition regime between giant planets (GPs) and brown dwarfs (BDs) is still an open subject of study in exoplanetary science. A complete understanding of the population of long-period GPs and BDs would be pivotal for improving our knowledge of this topic, but the number of such object...

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Principais autores: Pinamonti M., Sozzetti A., Barbato D., Desidera S., Biazzo K., Bonomo A. S., Lanza A. F., Naponiello L., Affer L., Anche R. M., Andreuzzi G., Basilicata M., Brinjikji M., Brogi M., Cabona L., Carolo E., Colombo S., Damasso M., D’Arpa M., Di Filippo S., Harutyunyan A., Hom J., Mancini L., Mantovan G., Nardiello D., Santhakumari K. K. R., Zingales T.
Format: Artigo
Sprog:Inglês
Udgivet: EDP Sciences 2026-03-01
Serier:Astronomy & Astrophysics
Fag:
methods: data analysis
techniques: radial velocities
astrometry
planets and satellites: individual: hd 118717 b
brown dwarfs
planetary systems
Online adgang:https://www.aanda.org/articles/aa/full_html/2026/03/aa57414-25/aa57414-25.html
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