Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date
Context. An accurate characterization of the known exoplanet population is key to understanding the origin and evolution of planetary systems. Determining true planetary masses through the radial velocity (RV) method is expected to experience a great improvement thanks to the availability of ultra-stable echelle spectrographs. Aims: We took
Toledo-Padrón, B. et al.
Fecha de publicación:
9
2020