Spectral energy distributions and luminosities of M dwarfs in the CARMENES search for exoplanets
In the quest for Earth-sized exoplanets, M dwarfs are stars of increasing interest during the last two decades. Their small sizes and masses as compared to our Sun make them specially suitable targets to look for the signatures of planetary companions, as their habitable zones fall closer to their host star. Despite being the most abundant stars in
Cifuentes, C. et al.
Fecha de publicación:
3
2019