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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 14.

Estimated posterior probability densities used to determine the global maxima corresponding to the rotation period in the HARPS radial velocities of GJ 674. The signal of GJ 674b has been accounted for, and the red arrows indicate the positions of the most prominent secondary maxima. The aperture ranges correspond to the four redmost sets of 12 HARPS orders.

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