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

Author(s):
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.
Published
2022
Publication type
Article / Letter to editor
Planets and satellites - detectionPlanets and satellites - dynamical evolution and stabilityPlanets and satellites - fundamental parametersAstrophysics - earth and planetary astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 515, no. 1, p. 1328-1345
hdl
1887/3515425
doi
10.1093/mnras/stac1383
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.1328D