Table 3
Accretion luminosities and mass accretion rates.
| Name | Template | BJobs | BJintr |
|
log Lacc,c | log Ṁacc,c |
| (L⊙) | (M⊙/yr) | |||||
|
|
||||||
| SO397 | SO797 | 0.85 | 1.9 | 0.16 | –2.71 | –9.42 |
| SO490 | SO797 | 1.50 | 10.4 | 0.36 | –3.10 | –9.97 |
| SO500 | SO925 | 3.52 | 13.1 | 1.05 | –3.95 | –10.27 |
| SO587 | Sz94 | 0.50 | ... | >1.7 | <-4.00 | <–10.41 |
| SO646 | Sz94 | 1.23 | 14.4 | 0.20 | –3.00 | –9.68 |
| SO848 | Sz94 | 2.72 | 14.4 | 0.43 | –3.50 | –10.39 |
| SO1260 | Sz94 | 1.61 | 1.38 | 0.12 | –2.00 | –8.97 |
| SO1266 | SO797 | 0.18 | ... | >1.8 | <–4.85 | <–11.38 |
Notes. Column 1 shows the name of the target, Col. 2 the name of the template used to compute the accretion luminosity. Columns 3 and 4 columns list the observed and the intrinsic Balmer jump. Column 5 lists the fraction of accretion luminosity contained in the Balmer series lines, and Lhigh − n BL refers to the luminosity of the Balmer lines at wavelengths shorter than λ375.0 nm. The last two columns represent the accretion luminosities and the mass accretion rates obtained from the excess continuum emission.
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