Table 9.

Dipper fractions for the three regions with well-studied dipper populations. The Upper Scorpius association and ρ Ophiuchus cluster have been added in this work. The dipper fraction quoted here is as a function of disc-bearing stars only.

RegionAgeDisc fractionDipper fractionDipper Number
ρ Ophiuchus0.1–1 Myr (Luhman & Rieke 1999)40.2 per cent ± 4.3 per cent20.1|$\,{\rm per \, cent} \pm 4.3\,{\rm per \, cent}$|22
NGC 22641–5 Myr (Rebull et al. 2002)Dahm (2008)12.8 per cent ± 1.0 per cent21.6|$\,{\rm per \, cent} \pm 3.7\,{\rm per \, cent}$| Cody et al. (2014)35
Upper Scorpius10 Myr (Pecaut et al. 2012)26.7 per cent ± 2.0 per cent21.8|$\,{\rm per \, cent} \pm 3.4\,{\rm per \, cent}$|42
RegionAgeDisc fractionDipper fractionDipper Number
ρ Ophiuchus0.1–1 Myr (Luhman & Rieke 1999)40.2 per cent ± 4.3 per cent20.1|$\,{\rm per \, cent} \pm 4.3\,{\rm per \, cent}$|22
NGC 22641–5 Myr (Rebull et al. 2002)Dahm (2008)12.8 per cent ± 1.0 per cent21.6|$\,{\rm per \, cent} \pm 3.7\,{\rm per \, cent}$| Cody et al. (2014)35
Upper Scorpius10 Myr (Pecaut et al. 2012)26.7 per cent ± 2.0 per cent21.8|$\,{\rm per \, cent} \pm 3.4\,{\rm per \, cent}$|42
Table 9.

Dipper fractions for the three regions with well-studied dipper populations. The Upper Scorpius association and ρ Ophiuchus cluster have been added in this work. The dipper fraction quoted here is as a function of disc-bearing stars only.

RegionAgeDisc fractionDipper fractionDipper Number
ρ Ophiuchus0.1–1 Myr (Luhman & Rieke 1999)40.2 per cent ± 4.3 per cent20.1|$\,{\rm per \, cent} \pm 4.3\,{\rm per \, cent}$|22
NGC 22641–5 Myr (Rebull et al. 2002)Dahm (2008)12.8 per cent ± 1.0 per cent21.6|$\,{\rm per \, cent} \pm 3.7\,{\rm per \, cent}$| Cody et al. (2014)35
Upper Scorpius10 Myr (Pecaut et al. 2012)26.7 per cent ± 2.0 per cent21.8|$\,{\rm per \, cent} \pm 3.4\,{\rm per \, cent}$|42
RegionAgeDisc fractionDipper fractionDipper Number
ρ Ophiuchus0.1–1 Myr (Luhman & Rieke 1999)40.2 per cent ± 4.3 per cent20.1|$\,{\rm per \, cent} \pm 4.3\,{\rm per \, cent}$|22
NGC 22641–5 Myr (Rebull et al. 2002)Dahm (2008)12.8 per cent ± 1.0 per cent21.6|$\,{\rm per \, cent} \pm 3.7\,{\rm per \, cent}$| Cody et al. (2014)35
Upper Scorpius10 Myr (Pecaut et al. 2012)26.7 per cent ± 2.0 per cent21.8|$\,{\rm per \, cent} \pm 3.4\,{\rm per \, cent}$|42
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