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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.