All Tables
- Table 1:
Data used for this analysis. Spectra
were taken with different high-resolution spectrographs.
Detection of differential rotation requires higher resolution in
slower rotators. The minimum rotation velocities required for
determining the rotation law are given in Col. 4. From the
147 spectra from which differential rotation could be determined, 28
stars show signatures of differential rotation.
- Table 2:
Amount of differential rotators, total number of stars, and percentage of differential rotators for each subsample of Fig. 1.
- Table 3:
Four stars with extreme values of differential
rotation
.
It is speculated that these objects represent a special class of targets (marked with downward arrows in Fig. 2) in a narrow region of rotation velocity and effective temperatures near the convection boundary.
- Table B.1:
Field stars with measured differential rotation.
- Table B.2:
Stars in cluster fields, FLAMES/UVES observations.