HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica

Dransfield, G.; Triaud, A.H.M.J.; Guillot, T.; Mekarnia, D.; Nesvorný, D.; Crouzet, N.M.; ... ; Zhou, G. (2022)

Article / Letter to editor

• Planets and satellites - detection
• Planets and satellites - dynamical evolution and stability
• Planets and satellites - fundamental parameters
• Astrophysics - earth and planetary astrophysics

• All authors: Dransfield, G.; Triaud, A.H.M.J.; Guillot, T.; Mekarnia, D.; Nesvorný, D.; Crouzet, N.M.; Abe, L.; Agabi, K.; Buttu, M.; Cabrera, J.; Gandolfi, D.; Günther, M.N.; Rodler, F.; Schmider, F.-X.; Stee, P.; Suarez, O.; Collins, K.A.; Dévora-Pajares, M.; Howell, S.B.; Matthews, E.C.; Standing, M.R.; Stassun, K.G.; Stockdale, C.; Quinn, S.N.; Ziegler, C.; Crossfield, I.J.M.; Lissauer, J.J.; Mann, A.W.; Matson, R.; Schlieder, J.; Zhou, G.
• Date: 2022
• Journal: Monthly Notices of the Royal Astronomical Society
• Volume: 515
• Issue: 1
• Pages: 1328 - 1345
• DOI: doi:10.1093/mnras/stac1383
• Link: https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.1328D