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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 7.

Left: on the top panel, [Fe/H] for single-transit planet hosts associated with each adjusted radius bin (purple). On the bottom panel, 〈e〉 vs. adjusted planet radius bin centers for the sample of M dwarf singles in this work (teal). Right: same as the left panel, but for multis.

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