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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 5.

RV, BIS SPAN, and FWHM variations and best fit (black continuous line) of the activity-induced signal observed on α Cen B. The best-fitted solution corresponds to a plage of size 2.4% that can be found at a latitude of 44 deg. The star rotates in 36.65 days and is seen with an inclination of 22 deg.

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