Densities of small planets around the M dwarfs TOI-4336 A and TOI-4342 with ESPRESSO: Three sub-Neptunes, one super-Earth, and a Neptune-mass candidate
Léna Romane Elisa Parc, Charles Cadieux, Nolan Grieves, F. Bouchy et autres
Context . Characterizing the masses, radii, and compositions of small planets orbiting M dwarfs is key to understanding their formation and identifying the best targets for atmospheric follow-up with facilities such as JWST. Aims . We present the characterization of two planetary …
ch, ca, pt, es, cl, fr, us, cn (code pays fourni par la source)
0 citations
Archive ouverte UNIGE (University of Geneva)