Table A.1
Mass accretion rates compiled from the literature.
| Source | log(M model) | Refs. | log(M v10) | Refs. |
|---|---|---|---|---|
| (M⊙ /yr) | (M⊙/yr) | |||
| RECX−1 | −11.9 | J06 | ||
| RECX−3 | −12.1* | L04 | −11.8* | J06 |
| RECX−4 | −11.9* | L04 | −11.5* | J06 |
| RECX−5 | −10.3 | L04 | −9.7,−11.0*,−9.89 | L04, J06, R18 |
| RECX−6 | −11.4* | L04 | −11.5* | J06 |
| RECX−7 | −11.7* | L04 | −10.1 | J06 |
| RECX−9 | −10.4 | L04 | −10.0,−9.1,−9.92 | L04, J06, R18 |
| RECX−10 | −11.8*,−11.9* | L04, J06 | ||
| RECX−11 | −10.4,−9.77 | L04,I13 | −−−9.7− -9.5− -9.49 | L04, J06, R18 |
| RECX−12 | −11.3*, −11.4* | L04J06 | ||
| ECHAJ0843 | −9.0,−9.10 | L04, I13 | −7.7,−8.7,−9.12 | L04, J06 |
| ECHAJ0844 | −10.18 | R18 | ||
| 2MASSJ0801 | −11.3*, −9.7 | M11 | ||
| 2MASSJ0820 | −10.6, −9.7 | M11 | −8.7 | M11 |
Notes. The accretion rates labeled Ṁmodel are derived from magnetospheric accretion model fits, while the rates labeled ṀV10 are from the relation between accretion rate and the Hα line width at 10% of the maximum (V10), from Natta et al. (2004). The uncertainties in the disk mass include detection and calibration uncertainties. ECHA 0841 has TO/flat SED, EW(Ha) = −12 AA. ECHA 0844 has flat SED and is likely accreting with EW(Ha) = −58 AA References: J06: Jayawardhana et al. (2006); L04: Lawson et al. (2004); M11: Murphy et al. (2013); I13: Ingleby et al. (2013); R18: Rugel et al. (2018); * = V10 below 200 km s-1, which is the minimum for the Natta et al. (2004) relation.
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