Table 3
Model properties.
| Model | BD | VLM stars | |||||||||
|
|
|||||||||||
|
σd |
|
σdl | tth |
|
σd |
|
σdl | tth | D-L | |
| (days) | (dex) | (days) | (dex) | (Myr) | (days) | (dex) | (days) | (dex) | (Myr) | (Y/N) | |
|
|
|||||||||||
| M1 | 1.0 | 3.0 | 1.0 | 3.0 | 2.2 | 2.0 | 4.0 | 2.0 | 4.0 | 2.2 | Y |
| M2 | 1.0 | 3.0 | 1.0 | 3.0 | 2.2 | 3.0 | 4.0 | 2.0 | 2.0 | 2.2 | Y |
| M3 | 1.0 | 3.0 | 1.0 | 3.0 | 2.2 | 2.0 | 4.0 | 2.0 | 4.0 | 4.2 | Y |
| M4 | 1.0 | 3.0 | 1.0 | 3.0 | 2.2 | 2.0 | 4.0 | 2.0 | 4.0 | 2.2 | N |
Notes.
,
and σd, σdl are the mean values and dispersions of the rotational period distributions of disk and diskless stars, respectively; tth is the threshold mass accretion rate time scale; and the D-L parameter specifies whether the model is taking into account the disk locking hypothesis (Y) or not (N).
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