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Table 1

Characteristics of the six subgiant and early red giant stars studied by Deheuvels et al. (2014).

M/M log  g ΔΩobs (μrad s-1)

1.22 3.83 ± 0.04 2.00 ± 0.66
1.27 3.77 ± 0.02 2.92 ± 0.79
1.14 3.76 ±0.04 4.65 ± 0.30
1.26 3.71 ± 0.03 9.04 ± 0.46
1.39 3.68 ± 0.02 7.48 ± 0.26
1.07 3.60 ± 0.02 9.31 ± 0.31

Notes. The mass were obtained with a fitting procedure using the evolution code CESTAM, log  g was determined by seismic scaling relations and the amplitude of the radial-differential rotation between the center of the star and the base of the convective zone was inferred from the OLA method.

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