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Table 6.
Literature age estimates for β Pic.
| Reference | Age | Method |
|---|---|---|
| Barrado y Navascués et al. (1999) | 20 ± 10 Myr | CMD isochronal age (KM stars) |
| Zuckerman et al. (2001) |
 Myr |
H–R diagram isochronal age (KM stars) |
| Ortega et al. (2002) | 11.5 Myr | Dynamical (Traceback) age |
| Song et al. (2003) | 12 Myr | Dynamical (Traceback) age |
| Ortega et al. (2004) | 10.8 ± 0.3 Myr | Dynamical (Traceback) age |
| Torres et al. (2006) | 18 Myr | Dynamical (Expansion) age |
| Makarov (2007) | 31 ± 21 Myr | Dynamical (Traceback) age |
| Mentuch et al. (2008) | 21 ± 9 Myr | Li depletion |
| Macdonald & Mullan (2010) | ∼40 Myr | Li depletion (magnetoconvection models) |
| Binks & Jeffries (2014) | 21 ± 4 Myr | Li depletion boundary |
| Malo et al. (2014b) | 26 ± 3 Myr | Li depletion boundary |
| Malo et al. (2014b) | 21.5 ± 6.5 Myr (15–28 Myr) | H–R diagram isochronal age (KM stars) |
| Mamajek & Bell (2014) | 22 ± 3 Myr | CMD isochronal age (FG stars) |
| Mamajek & Bell (2014) | 13 − 58 Myr | Dynamical (Expansion) age |
| Bell et al. (2015) | 24 ± 3 Myr | CMD isochronal age |
| Messina et al. (2016) | 25 ± 3 Myr | Li depletion boundary (rotation models) |
| Miret-Roig et al. (2018) |
 Myr |
Dynamical (Traceback) age |
| Crundall et al. (2019) |
 Myr |
Dynamical (Forward-modelling) age |
| Ujjwal et al. (2020) | 19.38 Myr (5.5 − 54.5 Myr) | CMD isochronal age |
| This work | 18.5 Myr |
Dynamical (Traceback) age |
Notes. This table is an udated version of Table 1 from Mamajek & Bell (2014).
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