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The Orbital Eccentricity–Radius Relation for Planets Orbiting M Dwarfs

  • Authors: Sheila Sagear, Sarah Ballard, Gregory J. Gilbert, Mariangel Albornoz, Christopher Lam

Sheila Sagear et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 13.

Same as Figure 2, but where 〈e〉 is calculated using the empirical eccentricity model rather than the beta distribution. The error bars represent the 16th and 84th percentiles of 〈e〉. The green histogram represents the number of M dwarf planets in each radius bin (right-hand vertical axis).

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