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Table H.1
Results of the power-law fits to the Mdust vs. M⋆ relations. The value of δ is a measure of the dispersion from the fit (see linmix documentation).
Mdust-M⋆ | Log10(Mdust/M⊙) = α + β * Log10Mstar/M⊙) | |||||
---|---|---|---|---|---|---|
α | β | Δ | α | β | δ | |
Region | full sample | M⋆≥ 0.15M⊙ | ||||
Corona Australis | 0.4±0.4 | 1.3±0.5 | 1.1±0.7 | 0.3±0.4 | 1.1±0.8 | 1.1±0.8 |
Taurus | 1.1±0.1 | 1.5±0.2 | 0.8±0.3 | 1.2±0.1 | 1.6±0.3 | 0.9±0.3 |
L1688 | 1.0±0.1 | 1.5±0.2 | 0.8±0.3 | 1.1±0.2 | 1.9±0.4 | 0.9±0.4 |
Lupus | 1.4±0.2 | 1.7±0.3 | 0.7±0.3 | 1.5±0.2 | 1.7±0.3 | 0.7±0.3 |
Chamaeleon I | 1.1±0.2 | 1.6±0.3 | 0.7±0.4 | 1.1±0.2 | 1.2±0.3 | 0.7±0.4 |
Upper Scorpius | 0.8±0.2 | 2.2±0.3 | 0.7±0.3 | 0.8±0.2 | 2.2±0.4 | 0.7±0.4 |
Macc-M⋆ | Log10(Ṁacc/(M⊙/yr)) = α + β * Log10(Mstar/M⊙) | |||||
α | β | Δ | α | β | δ | |
Region | full sample | M⋆≥ 0.15M⊙ | ||||
Corona Australis | – | – | – | – | – | – |
Taurus | – | – | – | – | – | – |
L1688 | −8.3±0.3 | 1.8±0.5 | 1.2±0.7 | −8.3±0.3 | 1.7±0.7 | 1.2±0.7 |
Lupus | −8.5±0.2 | 1.6±0.3 | 0.7±0.3 | −8.6±0.2 | 1.2±0.4 | 0.7±0.4 |
Chamaeleon I | −8.1±0.2 | 2.3±0.3 | 1.0±0.4 | −8.2±0.2 | 1.3±0.4 | 1.0±0.5 |
Upper Scorpius | −9.0±0.5 | 1.5±0.8 | 1.3±0.8 | −9.0±0.5 | 1.5±0.9 | 1.4±0.8 |
Ṁacc-Mdisk | Log10(Ṁacc/(M⊙/yr)) = α + β * Log10(Mdisk/M⊙) | |||||
α | β | Δ | α | β | δ | |
Region | full sample | M⋆ ≥ 0.15M⋆ | ||||
Corona Australis | – | – | – | – | – | – |
Taurus | – | – | – | – | – | – |
L1688 | −6.0±0.5 | 1.0±0.2 | 0.9±0.5 | −6.2±0.6 | 0.9±0.2 | 0.9±0.6 |
Lupus | −7.2±0.4 | 0.7±0.2 | 0.7±0.4 | −7.6±0.4 | 0.6±0.2 | 0.7±0.3 |
Chamaeleon I | −6.0±0.6 | 1.1±0.2 | 1.1±0.5 | −6.6±0.6 | 0.7±0.2 | 1.0±0.5 |
Upper Scorpius | −7.0±1.3 | 0.8±0.4 | 1.3±0.7 | −7.0±1.4 | 0.8±0.4 | 1.3±0.8 |
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