Table B.1.
Summary of the line parameters of the common accretion tracers.
| Line Tracer | λ [nm] | Lacc Outburst | Ṁ Outburst [M⊙yr−1] | Ṁ Quiescent [M⊙yr−1] |
|---|---|---|---|---|
| Hα | 656.3 | 3.51 ± 3.24 × 10−4 | 4.96 ± 1.94 × 10−10* | 5.32 ± 2.37 × 10−11 |
| Hβ | 486.1 | 7.39 ± 0.88 × 10−6 | 1.05 ± 1.30 × 10−11* | ** |
| Hγ | 434.1 | 5.66 ± 1.26 × 10−8 | 8.01 ± 1.34 × 10−14* | ** |
| Paβ | 1281.8 | 1.98 ± 0.56 × 10−1 | 2.80 ± 0.85 × 10−7 | 6.29 ± 1.81 × 10−9 |
| Paγ | 1093.8 | 6.55 ± 0.19 × 10−2 | 9.27 ± 0.0.61 × 10−8 | 2.50 ± 1.81 × 10−9 |
| Paδ | 1004.9 | 8.73 ± 0.29 × 10−2 | 1.23 ± 1.25 × 10−7 | 7.87 ± 1.61 × 10−10 |
| Pa8 | 954.6 | 5.03 ± 0.15 × 10−2 | 7.12 ± 0.38 × 10−8 | 2.26 ± 1.59 × 10−9 |
| Pa9 | 922.9 | 5.66 ± 0.13 × 10−2 | 8.00 ± 0.42 × 10−8 | 6.38 ± 1.48 × 10−11 |
| Pa10 | 901.5 | 3.96 ± 0.13 × 10−2 | 5.60 ± 0.44 × 10−8 | 1.43 ± 0.94 × 10−10 |
| Brγ | 2165.3 | 1.02 ± 0.03 | 1.44 ± 0.19 × 10−6 | 3.57 ± 2.51 × 10−8 |
| Br(11 − 4) | 1680.6 | 3.78 ± 0.03 × 10−2 | 3.73 ± 0.25 × 10−7 | ** |
| Br(12 − 4) | 1640.7 | 3.26 ± 0.02 × 10−2 | 3.25 ± 0.28 × 10−7 | ** |
| Br(13 − 4) | 1610.9 | 5.34 ± 0.04 × 10−2 | 5.29 ± 0.35 × 10−7 | ** |
| Br(14 − 4) | 1588.0 | 5.70 ± 0.06 × 10−2 | 3.43 ± 0.24 × 10−7 | ** |
| Br(15 − 4) | 1570.1 | 5.61 ± 0.05 × 10−2 | 5.55 ± 0.42 × 10−7 | ** |
| Br(16 − 4) | 1555.6 | 5.56 ± 0.04 × 10−2 | 3.81 ± 0.29 × 10−7 | ** |
| Br(17 − 4) | 1543.9 | 5.40 ± 0.05 × 10−2 | 3.47 ± 0.25 × 10−7 | ** |
| HeI | 1082.9 | 3.31 ± 0.40 × 10−2 | 4.69 ± 0.38 × 10−8 | 1.24 ± 1.15 × 10−10 |
| HeI | 587.6 | 1.21 ± 1.47 × 10−4 | 1.71 ± 1.16 × 10−10 | 2.92 ± 2.28 × 10−12 |
| CaII | 849.8 | 4.29 ± 0.55 × 10−2 | 6.07 ± 0.61 × 10−8 | 7.41 ± 1.01 × 10−10 |
| CaII | 854.2 | 6.97 ± 0.14 × 10−2 | 9.87 ± 0.78 × 10−8 | 2.83 ± 1.65 × 10−10 |
| CaII | 866.2 | 1.09 ± 0.18 × 10−1 | 1.54 ± 0.41 × 10−7 | 1.28 ± 0.87 × 10−9 |
Notes. EW is the line equivalent width, Lacc is the associated accretion luminosity, and Ṁ is the calculated accretion rate.
Measurements are strongly impacted by p-cyngi profiles in the line; as such, they are not considered when computing the final accretion rate.
Line too faint for accurate measurements.
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