Table 3
Six sets of parameters for which the theoretical K-P relation has been calculated.
| Model | C 1 | α h | R d,max | M 1 | ||||||
|
|
||||||||||
| 1 | −2.5 | 0.01 | 2 | 1 | ||||||
| 2 | −0.95 | 0.2 | 0.6 | 0.6 | ||||||
| 3 | −0.2 | 0.2 | 2 | 1 | ||||||
| 4* | 0.1 | 0.2 | 0.7 | 1 | ||||||
| 5 | 1.2 | 0.2 | 5 | 1.2 | ||||||
| 6* | 1.3 | 0.2 | 0.8 | 1.2 | ||||||
Notes. αh – hot disc viscosity parameter, and C1 – the constant from Eq. (17) calculated for a given set of parameters. Models 2 and 5 correspond to the lower and upper limits of the theoretical K-P relation for solar discs with αh = 0.2;
models are calculated for helium discs (Y = 0.98 Z = 0.02): model 4 ∗ gives the K-P relation for PTF1J0719, model 6 ∗ gives the K-P relation for CR Boo and V803 Cen in their cycling states. The models are plotted with lines in Fig. 5.
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