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Table 5
Estimated magnetic field strength on the line-of-sight Blos, its uncertainty, strength of the magnetic field extrapolated (following a 1 /r law) at one stellar radius (see Sect. 6) Br∗, and instrumental contribution parameters C1 and C2 for each object in our sample.
| Object | B los | δ B los | B r ∗ | | C1 | | C 2 |
| [mG] | [mG] | [G] | × 10-3 | [Hz] | |
|
|
|||||
| RW LMi | ≤ 3.8 | ≤ 4.4 | 1.05 | 9200 | |
| RY Dra | ≤ 14.2 | ≤ 4.8 | 1.15 | 17 500 | |
| AFGL618 | 6.0 | 6.0 | 67.5 | 1.05 | 2750 |
| NGC 7027 | ≤ 8.0 | ≤ 3.1 × 105 | 1.1 | 1360 | |
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