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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 9.

HARPS radial velocities of AD Leo between JDs 2453809.7 and 2453871.6 as a function of time (top panel) and folded on the phase of the signal (bottom panel). The black curve denotes the estimated Keplerian curve. The three temporal subsets of data denoted by different colors have been treated as independent data sets with independent nuisance parameters.

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