DREAM - II. The spin–orbit angle distribution of close-in exoplanets under the lens of tides

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Table 1

Tabulated values of the mass of the stellar convective envelope, used to compute the tidal efficiency factor, as a function of the stellar mass.

M_⋆ [M_⊙]	log T_eff [K]	Mconv/M_⋆
0.5	3.60337	0.3508
0.6	3.62040	0.1842
0.7	3.64646	0.0991
0.8	3.68716	0.0667
0.9	3.72492	0.0437
1.0	3.75427	0.0257
1.1	3.77156	0.0107
1.2	3.79455	0.0031
1.3	3.81339	0.0003
1.4	3.83224	0.0000
1.5	3.85367	0.0000

Notes. The stellar effective temperature, as generated by our model, is given for indicative purposes. In particular, one can see that M_conv/M_⋆ drops below 1% at roughly the temperature of the Kraft break.

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