Fig. 11
Properties of RV exoplanets orbiting M dwarfs. Top-left panel: orbital period as a function of the mass of the host star. Top-right panel: orbital period as a function of the metallicity of the host star. Bottom-left panel: minimum mass as a function of the mass of the host star. Bottom right panel: minimum mass as a function of the metallicity of the host star. The red dots represent the M-dwarf hosted RV extrasolar planets, the blue dots represent the HADES planets, and the blue star represents the newly detected planet GJ 685 b.
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