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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 3.

Correlation between the different posterior distributions obtained from the MCMC fit to the data of HD 189733 constraining α and γ so that the spot is on the northern hemisphere and cannot grow in size on the hidden part of the star. The 1σ and 2σ contours are shown in dashed red and continuous green lines, respectively.

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