Table 6
Line luminosities and derived accretion luminosities for Cha II objects (see caption of Table 5).
| Id | L [O] i | L Ca ii | L Hα | L Paβ | L Brγ | L acc [O] i | L acc Ca ii | L acc Hα | L acc Paβ | L acc Brγ | Ṁ acc Brγ |
| Cha II | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | L ⊙ | M⊙ yr-1 |
|
|
|||||||||||
| 1a | 1.54 × 10-1 | 9.51 × 10-2 | 6.34 × 10-1 | 1.81 × 10-3 | 6.12 × 10-3 | 1.05 × 102 | 2.87 × 101 | 1.05 × 102 | 6.58 | 8.10 | 4.49 × 10-7 |
| 2 | <1.89 × 10-4 | <2.39 × 10-4 | 4.77 × 10-4 | <9.19 × 10-5 | 7.53 × 10-5 | <1.68 × 10-1 | <6.39 × 10-2 | 1.31 × 10-2 | <7.86 × 10-2 | 1.55 × 10-1 | 1.60 × 10-8 |
| 3 | ... | ... | ... | ... | 1.92 × 10-3 | ... | ... | ... | ... | 2.85 | 9.10 × 10-7 |
| 4 | ... | ... | 7.87 × 10-4 | 8.35 × 10-5 | 2.11 × 10-5 | ... | ... | 2.46 × 10-2 | 5.90 × 10-2 | 4.91 × 10-2 | 2.70 × 10-9 |
| 5 | <4.25 × 10-5 | <4.41 × 10-5 | 9.04 × 10-5 | 1.50 × 10-5 | 4.12 × 10-5 | <4.01 × 10-2 | <1.14 × 10-2 | 1.64 × 10-3 | 1.33 × 10-2 | 8.99 × 10-2 | 6.42 × 10-9 |
| 6 | <1.27 × 10-4 | 2.91 × 10-4 | 9.65 × 10-3 | 2.95 × 10-5 | 1.11 × 10-4 | <1.15 × 10-1 | 7.83 × 10-2 | 5.63 × 10-1 | 2.62 × 10-2 | 2.19 × 10-1 | 5.42 × 10-8 |
| 7 | <5.60 × 10-5 | 7.44 × 10-5 | 2.67 × 10-3 | <5.94 × 10-5 | 4.85 × 10-5 | <5.23 × 10-2 | 1.95 × 10-2 | 1.13 × 10-1 | <3.64 × 10-2 | 1.04 × 10-1 | 6.45 × 10-9 |
| 8 | <1.84 × 10-5 | <1.67 × 10-5 | 6.24 × 10-4 | 3.18 × 10-5 | 1.93 × 10-5 | <1.80 × 10-2 | <4.23 × 10-3 | 1.84 × 10-2 | 1.64 × 10-2 | 4.53 × 10-2 | 4.50 × 10-9 |
| 9 | <3.84 × 10-5 | <8.19 × 10-5 | 3.38 × 10-4 | 3.20 × 10-5 | 4.82 × 10-5 | <3.64 × 10-2 | <2.14 × 10-2 | 8.55 × 10-3 | 1.83 × 10-2 | 1.03 × 10-1 | 4.73 × 10-9 |
| 10 | <8.49 × 10-5 | <1.32 × 10-4 | 5.58 × 10-4 | <5.63 × 10-5 | 5.48 × 10-5 | <7.80 × 10-2 | <3.49 × 10-2 | 1.60 × 10-2 | <4.28 × 10-2 | 1.16 × 10-1 | 1.10 × 10-8 |
| 11 | 1.35 × 10-4 | 1.01 × 10-4 | 2.50 × 10-3 | 5.97 × 10-5 | 2.78 × 10-5 | 1.22 × 10-1 | 2.65 × 10-2 | 1.04 × 10-1 | 5.33 × 10-2 | 6.31 × 10-2 | 4.68 × 10-9 |
| 12 | 2.83 × 10-5 | <5.54 × 10-5 | 5.92 × 10-4 | 2.74 × 10-5 | 1.22 × 10-5 | 2.72 × 10-2 | <1.44 × 10-2 | 1.72 × 10-2 | 2.19 × 10-2 | 3.01 × 10-2 | 7.16 × 10-9 |
| 13 | 4.75 × 10-5 | <1.14 × 10-4 | 8.56 × 10-4 | <5.22 × 10-5 | 2.68 × 10-5 | 4.46 × 10-2 | <3.01 × 10-2 | 2.73 × 10-2 | <4.19 × 10-2 | 6.11 × 10-2 | 3.60 × 10-8 |
| 14 | <6.05 × 10-5 | 2.47 × 10-4 | 3.33 × 10-3 | 4.01 × 10-5 | 4.38 × 10-5 | <5.63 × 10-2 | 6.63 × 10-2 | 1.49 × 10-1 | 3.65 × 10-2 | 9.49 × 10-2 | 4.53 × 10-9 |
| 15 | 1.66 × 10-4 | 2.96 × 10-4 | 1.48 × 10-2 | 4.55 × 10-4 | 2.02 × 10-4 | 1.48 × 10-1 | 7.95 × 10-2 | 9.63 × 10-1 | 3.92 × 10-1 | 3.76 × 10-1 | 2.01 × 10-8 |
| 16 | <3.21 × 10-5 | <3.63 × 10-5 | 8.89 × 10-5 | 3.66 × 10-5 | 2.38 × 10-5 | <3.06 × 10-2 | <9.36 × 10-3 | 1.61 × 10-3 | 2.52 × 10-2 | 5.49 × 10-2 | 3.02 × 10-9 |
| 17 | 1.17 × 10-5 | 2.21 × 10-5 | 4.63 × 10-4 | <7.43 × 10-5 | <2.49 × 10-5 | 1.16 × 10-2 | 5.65 × 10-3 | 1.27 × 10-2 | <3.78 × 10-2 | <5.71 × 10-2 | <5.49 × 10-9 |
Notes. The mass accretion rates are computed from the the Brγ accretion luminosity, using the available stellar parameters given in Table 2.
A more detailed analysis of ChaII-1 (DK Cha) is presented in García López et al. (2011).
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