Figure 6 from Deriving Stellar Inclination of Slow Rotators Using Stellar Activity

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Deriving Stellar Inclination of Slow Rotators Using Stellar Activity

Authors: X. Dumusque

Dumusque 2014 The Astrophysical Journal 796 133.

Provider: AAS Journals

Caption: Figure 6.

Correlation between the different posterior distributions obtained from the MCMC fit to the data of α Cen B. The 1σ and 2σ contours are shown with dashed red and continuous green lines, respectively.

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