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Table E.2.

Luminosities of other emission lines used as tracers of accretion, when detected.

Star LCa II λ3934 ± err LHe I λ4026 ± err LHe I λ5876 ± err LPaβ ± err
[ × 10−7L] [ × 10−7L] [ × 10−7L] [ × 10−7L]
TWA 1 [10 s] 460 ± 40 110 ± 50 360 ± 70 2320 ± 70
TWA 1 [60 s] 450 ± 30 90 ± 40 330 ± 130 2250 ± 100
TWA 3A 23 ± 3 6 ± 3
TWA 8A 135 ± 2 8 ± 5 21 ± 11
TWA 8B 9.6 ± 0.7 2.0 ± 0.9
TWA 22 5.4 ± 0.4 1.2 ± 0.3
TWA 27 [P084] 0.6 ± 0.2 0.20 ± 0.17
TWA 27 [P089] 0.21 ± 0.03 0.06 ± 0.02
TWA 28 0.51 ± 0.07
TWA 30A [P087, ns] 33 ± 12
TWA 30A [P087, ls] 20 ± 2
TWA 30A [P287] 18 ± 6 0.8 ± 0.2
TWA 30B [P087] 0.034 ± 0.004
TWA 30B [P287] 0.35 ± 0.09
TWA 31 15.1 ± 0.8 3.0 ± 0.7 11.1 ± 0.6 17.0 ± 1.9
TWA 32 12.5 ± 0.3 1.1 ± 0.2 6.2 ± 0.5
TWA 40
J1247-3816

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