Table 1
Best-fit parameters of the identified accretion-tracing lines.
| Line | Rest wavelengtha (Å) | Peak positionb (Å) | Velocity shift (km s−1) | FWHMc (km s−1) |
|---|---|---|---|---|
| Hβ | 4861.3 | 4861.1 | −17 ± 2 | 60 ± 2 |
| Hα | 6562.8 | 6562.6 | −9 ± 1 | 47 ± 1 |
| Ca II | 8498.0 | 8497.9 | +16 ± 2 | [231 ± 4, 82 ± 5] |
| Ca II | 8542.1 | 8541.9 | +16 ± 1 | [247 ± 2, 42 ± 3] |
| Ca II | 8662.1 | 8662.0 | +13 ± 1 | [253 ± 6, 40 ± 4] |
| Paδ | 10049.8 | 10049.04 | −13 ± 1 | [209 ± 8, 48 ± 2] |
| Paγ | 10938.1 | 10937.8 | −7 ± 1 | [245 ± 9, 32 ± 2] |
| Paβ | 12818.1 | 12817.7 | −10 ± 1 | [274 ± 5, 44 ± 1] |
| Brγ | 21655.3 | 21653.4 | −8 ± 1 | [200 ± 4, 20 ± 3] |
Notes. (a) The wavelengths are measured in air. (b) Where the line shows both double and narrow components, we report the peak position for the narrow component. (c) When the line exhibits both broad and narrow components, we report each FWHM separately. In such cases, the column contains two values within brackets, where the first value corresponds to the broad component and the second to the narrow component.
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