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Table B.1
Observability of young stars for some representative values assuming a lower limit to the stellar brightness in the R band of 13 mag.
| Sources at 150 pc | |||
|---|---|---|---|
| AV = 0.0 mag | AV = 2.0 mag | ||
| M* (M⊙) | Age (Myr) | M* (M⊙) | Age (Myr) |
| 0.2 | Never | 0.4 | Never |
| 0.3 | <2 | 0.5 | <1 |
| 0.4 | <3 | 0.6 | <2 |
| 0.5 | <6 | 0.7 | <3 |
| 0.6 | Always | 0.8 | Always |
| Sources at 300 pc | |||
| AV = 0.0 mag | AV = 2.0 mag | ||
| M* (M⊙) | Age (Myr) | M* (M⊙) | Age (Myr) |
| 0.4 | Never | 0.9 | Never |
| 0.5 | <1 | 1.0 | <2 |
| 0.6 | <2 | 1.1 | Always |
| 0.8 | <6 | ||
| 0.9 | Always | ||
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