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Table 1.
Values of core and envelope rotations rates in our initial rotation profiles.
| Profile | Ωcore/2π (μHz) | Ωenv/2π (μHz) |
|---|---|---|
| A | 1.00 | 0.05 |
| B | 0.60 | 0.05 |
| C | 0.60 | 0.10 |
| D | 0.35 | 0.05 |
Notes. Profiles A, B and C have core and envelope rotation rates compatible with observations of subgiant stars (Deheuvels et al. 2014). Profile D has a core rotation rate lower than observations.
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