Table 4
Properties of the sources showing lithium EW variability.
| Object | SpT | INS | Binarity1 | IR Class | Teff2 | vsini3 | Hα Vble4 | X-ray5 |
|
|
||||||||
| LOri013 | M3.5 | (8) | III | 3750 | – | – | Y | |
| LOri045 | M3 | (8) (6) | III | 3500 | <17 | Y | N | |
| LOri057 | M5.5 | (3) | III | 3700 | <17.0 | N | N | |
| LOri063 | M4.0 | (3) | II | 3700 | <18.2 | Y | N | |
| LOri068 | M4.5 M5.0 | (1) (3) | III | 3700.0 | <17.0 | Y | N | |
| LOri075 | M5.0 M5.5 | (2) (8) (3) | SB1 (M08) | III | 3400 |
|
Y | N |
| LOri088 | M5.5 | (8) | III | 3200 | <17.0 | Y | N | |
| LOri094 | M5.5 | (8) (1) | III | 3200.0 |
|
Y | N | |
| LOri106 | M5.5 | (1) | II | 3200 | <17.0 | Y | N | |
Notes. (Sacco et al. 2008; Dolan & Mathieu 1999, 2001 values compared to the values derived in this work, third column.) Note that there is no bias in terms of the resolution of the spectra (as we also proved with the exercise of Appendix A). The instrument code is the same as in Table 6.
According to Sacco et al. (2008) (S08) or Maxted et al. (2008) (M08).
From Sacco et al. (2008).
Comparing the measurements of this work (see Paper II) and/or with those of Sacco et al. (2008).
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