Table 2
Ratio between the expected radius ℛ and the theoretical average radius ⟨R⟩ in a ΔM ≈ 0.2 M⊙ bin centred on M ≈ 0.7 M⊙ for stars not belonging to the slow-rotator sequence and P > 2 d.
| Set | ⟨M⟩ | n | nul |  /⟨Rtheo⟩ |
σ/⟨Rtheo⟩ |
|
|
|||||
| All | 0.68 | 41 | 5 |
|
0.19 |
| Q98 | 0.71 | 24 | 0 |
|
0.17 |
| T00 | 0.65 | 13 | 3 |
|
0.12 |
Notes. Calculations are carried out using all vsini values, only the Queloz et al. (1998)vsini (Q98), and only the Terndrup et al. (2000)vsini (T00). n is the number of points in the bin, nul the number of vsini upper limits. The estimated uncertainties due to SDR are reported together with ℛ/⟨Rtheo⟩, with a separate column for the standard deviation σ scaled by ⟨Rtheo⟩.
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