Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS
Ares Osborn, Ryan Cloutier, Vincent Bourrier, Bennett N. Skinner et autres
The Neptunian desert is a distinct lack of Neptune-sized planets at short orbital periods, purportedly carved by photoevaporation and tidal circularisation following high-eccentricity migration. Constraining these processes and how they vary across different hoststar spectral types requires detailed characterisation of the planets …
fr, gb, ca, ch, es, pt, br, us, cl, au, de (code pays fourni par la source)
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Astronomy and Astrophysics