The Rossiter-McLaughlin effect reloaded: Probing the 3D spin-orbit geometry, differential stellar rotation, and the spatially-resolved stellar spectrum of star-planet systems

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Table 4

Previous v_eq sin i_⋆ reported for HD 189733.


v_eq sin i_⋆ (km s^-1)	Method	Reference


3.5 ± 1	Line Broadening	Bouchy et al. (2005)
2.97 ± 0.22	Model Star	Winn et al. (2006)
3.2 ± 0.7	Line Broadening	Winn et al. (2006) ^a
3.316	Model Star	Triaud et al. (2009)
3.05	Model Star^b	Triaud et al. (2009)
3.08−3.1 ± 0.02^c	Tomography	Collier Cameron et al. (2010)
3.41 ± 0.02 ^d	Polarimetry	Fares et al. (2010)

Notes.

^(a)

D. Fischer (2006).

^(b)

Adjusted to reduce trend in residuals.

^(c)

Exact result was limb darkening and transit dependent.

^(d)

Converted from their reported equotorial period, under their assumption i_⋆ ≈ i_p.

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