Table 4
Magnetic field measurement results.
| Star | ⟨ B ⟩ 3 | ⟨ B ⟩ 1.5 | ||||||
| (kG) | (kG) | |||||||
| min | best | max | min | best | max | |||
|
|
||||||||
| CHXR 28 | 1.3 | 1.5 | 1.7 | 2.2 | 2.4 | 2.7 | ||
| YLW 19 | 0.2 | 0.8 | 1.0 | 0.0 | 1.7 | 2.4 | ||
| COUP 107 | – | – | – | 1.7 | 1.9 | 2.2 | ||
| V2062 Oph | 1.4 | 1.8 | 2.2 | 1.2 | 2.7 | 3.6 | ||
| V1149 Sco | 1.1 | 1.4 | 1.7 | 1.3 | 1.9 | 2.2 | ||
| Par 2441 | 0.5 | 0.8 | 1.0 | 0.4 | 1.6 | 2.2 | ||
Notes. The magnetic field has been estimated using 2 sets of spectral lines: ⟨ B ⟩3 with geff = 3 Fe i 15 648.5 Å, and ⟨ B ⟩1.5 with geff = 1.5 Fe i 15 622 Å and 15 662 Å. Columns 3 and 6 indicate the magnetic field values yielding the best fit to the spectral lines, while Cols. 2 and 5 and Cols. 4 and 7 respectively give the 1σ lower and upper limits.
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