TOI-1670 b and c: an inner sub-Neptune with an outer warm Jupiter unlikely to have originated from high-eccentricity migration

Author(s):
Tran, Q.H.; Bowler, B.P.; Endl, M.; Cochran, W.D.; MacQueen, P.J.; Gandolfi, D.; Persson, C.M.; Fridlund, M.; Palle, E.; Nowak, G.; Deeg, H.J.; Luque, R.; Livingston, J.H.; Kabáth, P.; Skarka, M.; Šubjak, J.; Howell, S.B.; Albrecht, S.H.; Collins, K.A.; Esposito, M.; Van Eylen, V.; Grziwa, S.; Goffo, E.; Huang, C.X.; Jenkins, J.M.; Karjalainen, M.; Karjalainen, R.; Knudstrup, E.; Korth, J.; Lam, K.W.F.; Latham, D.W.; Levine, A.M.; Osborne, H.L.M.; Quinn, S.N.; Redfield, S.; Ricker, G.R.; Seager, S.; Serrano, L.M.; Smith, A.M.S.; Twicken, J.D.; Winn, J.N.
Published
2022
Publication type
Article / Letter to editor
Exoplanet astronomyRadial velocityExoplanet formationTransit photometry48613324921709Astrophysics - Earth and Planetary Astrophysics
Date issued
2022
Language
English
Is part of
The Astronomical Journal (2022), No. 5, 225
hdl
1887/3561576
doi
10.3847/1538-3881/ac5c4f
URL
https://ui.adsabs.harvard.edu/abs/2022AJ....163..225T