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AD Leonis: Radial Velocity Signal of Stellar Rotation or Spin–Orbit Resonance?

  • Authors: Mikko Tuomi, Hugh R. A. Jones, John R. Barnes, Guillem Anglada-Escudé, R. Paul Butler, Marcin Kiraga, and Steven S. Vogt

2018 The Astronomical Journal 155 192.

  • Provider: AAS Journals

Caption: Figure 6.

Estimated posterior density as a function of the signal period given the HARPS and HIRES radial velocities of AD Leo. The horizontal lines represent the 10% (dotted), 1% (dashed), and 0.1% (solid) equiprobability thresholds with respect to the global maximum denoted by the red arrow.

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