Table 5.
Veiling and accretion rates for spectroscopic candidates.
| Gaia ID | Sp. | Veiling | Ṁ |
|---|---|---|---|
| Type | r7465 | (M⊙ yr−1) | |
| 2178495549568315776 | K6.6 | 0.41 | 6×10−9 |
| 2178296744121734912 | K7.4 | 0.33 | 4×10−9 |
| 2178450160360276480 | K8.0 | 0.27 | 8×10−9 |
| 2179207998742440960 | K8.2 | 0.09 | 4×10−9 |
| 2178432671252489984 | M2.6 | 0.12 | 6×10−9 |
| 2178458986501139840 | M3.0 | 0.73 | 7×10−9 |
| 2178433805123877504 | M3.6 | 0.23 | 5×10−9 |
| 2178433942562827136 | M3.6 | 0.23 | 6×10−9 |
| 2178547776372232704 | M4.0 | 0.86 | 4×10−8 |
| 2178385838927821440 | M4.2 | 0.15 | 3×10−9 |
| 2179218096198430848 | M4.4 | 0.83 | 9×10−9 |
| 2178434148721240320 | M4.8 | 0.55 | 7×10−9 |
| 2178444177454554496 | M4.8 | 0.64 | 5×10−8 |
| 2178443254045917568 (*) | M5.6 | 1.95 | 4×10−7 |
| 2178385735848603776 | M5.0 | 0.38 | 8×10−9 |
| 2178393771716897536 | M2.2 | 0.26 | 5×10−9 |
| 2178421671829472256 | M6.2 | 0.72 | 2×10−8 |
| 2179285376874962304 (*) | K0.0 | 2.58 | 7×10−7 |
| 2178441604784967168 (* *) | K9.6 | 0.09 | 6×10−9 |
| 2179215832763067648 | M2.6 | 0.17 | 4×10−9 |
| 2178398070997784960 | M3.2 | 0.97 | 2×10−8 |
| 2179216824887982592 | M3.6 | 0.30 | 7×10−9 |
| 2178434767196685440 | M4.0 | 0.53 | 1×10−8 |
| 2179224212235705344 (* *) | M4.2 | 0.13 | 1×10−8 |
| 2178441428675371136 (* *) | M5.2 | 0.13 | 2×10−8 |
Notes. (*)Sources with uncertain veiling measurements. The M5.6 source has a low S/N spectrum, so the veiling measurement is uncertain. The K0.0 source has good S/N, but the spectral type is uncertain, and so is the veiling.
(* *)Sources with a low S/N spectrum, so their veiling measurements and accretion rates are uncertain.
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