Table 1.
DIB's EWs identified in the early spectra of V1369 Cen.
| DIB | EW | Epoch | E(B−V) | Ref. |
|---|---|---|---|---|
| (nm) | (mÅ) | (days) | (mag) | |
| 578.0 | 140 ± 7 | 13 | 0.27 ± 0.02 | (Yuan & Liu 2011) |
| 578.0 | 140 ± 7 | 13 | 0.31 ± 0.07 | (Raimond et al. 2012) |
| 578.0 | 140 ± 7 | 13 | 0.26 ± 0.02 | (Munari & Zwitter 1997) |
| 661.4 | 72 ± 12 | 13 | 0.70 ± 0.10 | (Yuan & Liu 2011) |
| 661.4 | 72 ± 12 | 13 | 0.35 ± 0.09 | (Raimond et al. 2012) |
| 862.1 | 75 ± 4 | 7 | 0.29 ± 0.06 | (Puspitarini et al. 2015) |
Notes. In the first two columns, we present measurements of the DIB's EWs in the early optical spectra of V1369 Cen. The precise epoch of these measurements is reported in the third column. Corresponding E(B-V) values are provided in the fourth column, while the last column indicates the reference for the methodology used to measure the colour excess.
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