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Table 2
Values for projected stellar rotation rate, spin-orbit misalignment angle and width of the intrinsic stellar line profile compared to those from the two previous Rossiter-McLaughlin studies of WASP-3b.
| Parameter | Simpson et al. (2009) | Tripathi et al. (2010) | This study | Units |
|
|
||||
| vsini |
|
|
|
km s-1 |
| λ |
|
|
|
degrees |
| vg | Used result from this study | NA |
|
km s-1 |
Notes. The value obtained for vsini through spectral analysis is 13.4 ± 1.5 km s-1 (Pollacco et al. 2008).
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