eccentric planets
eccentric planets
eccentric planets
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Influence of the host star mass<br />
•Equal bin in log(Mstar)<br />
• M dwarfs<br />
• solar stars<br />
• intermediate masses<br />
•Planetary system mass / star number<br />
=> mass of planetary material scales with<br />
Mstar<br />
•Planets around more massive stars are<br />
more massive and more frequent.<br />
•RV bias underestimate the last bin.<br />
•The Neptunian vs Jovian planet ratio is<br />
higher around M dwarfs.<br />
•Consistent with a correlation of stellar<br />
mass, protoplanetary disk mass, and<br />
(giant) planet formation probability.
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