Table 5.
Polarization rates, angles, and magnetic field values for all components and all stars for the saturated and unsaturated cases.
| Star | # | pL | pC | χ | BE | BE (2nd solution) | BZ × cos(θ2) | Comment |
|---|---|---|---|---|---|---|---|---|
| (%) | (%) | (°) | (Gauss) | (Gauss) | (Gauss) | |||
| R Aql | 1 – a | 7.5 | –1.0 | 179.5 | (6.1 ± 2.0) | (3.7 ± 1.3) | (5.3 ± 1.8) | * |
| – b | 21.4 | 3.4 | 95.3 | (21.6 ± 7.3) | (9.8 ± 3.3) | (8.2 ± 2.8) | * | |
| μ Cep | 1 – a | 4.5 | –0.9 | 143.6 | (3.7 ± 3.4) | (2.4 ± 2.2) | (12.2 ± 11.1) | * |
| – b | 5.3 | 1.0 | 133.8 | (4.3 ± 3.9) | (2.7 ± 2.4) | (28.1 ± 25.6) | * | |
| 2 – a | 7.9 | 14.0 | 145.4 | (76.9 ± 49.4) | (43.3 ± 27.8) | (63.6 ± 40.1) | * | |
| – b | 8.1 | –1.8 | 117.6 | (10.4 ± 6.7) | (6.1 ± 3.9) | (9.9 ± 6.4) | * | |
| o Ceti | 1 – a | 58.9 | –2.2 | 147.5 | (8.0 ±2.1) | (40.0 ± 10.8) | * | |
| – b | 9.6 | 6.2 | 136.4 | (23.4 ± 6.3) | (13.2 ± 3.6) | (182.5 ± 49.5) | * | |
| 2 – a | 33.4 | 3.3 | 76.1 | 2.5 ± 0.4 | 2.7 ± 0.42 | |||
| – b | 15.9 | 0.8 | 77.1 | 1.6 ± 0.3 | 0.8 ± 0.1 | 5.2 ± 0.8 | ||
| 3 – a | 23.3 | 2.1 | 65.6 | 4.9 ± 0.5 | 2.1 ± 0.2 | 31.0 ± 3.4 | ||
| – b | 4.7 | –1.6 | 29.9 | 8.9 ± 1.0 | 5.8 ± 0.6 | 13.2 ± 1.5 | ||
| 4 – a | 4.7 | –1.6 | 29.9 | 4.2 ± 0.9 | 2.7 ± 0.8 | 7.0 ± 1.5 | ||
| – b | 29.6 | –2.2 | 33.9 | 4.0 ± 0.8 | 1.5 ± 0.3 | 5.7 ± 1.2 | ||
| 5 – a | 47.0 | –1.5 | 35.3 | 0.4 ± 0.2 | 1.0 ± 0.4 | |||
| – b | 52.6 | 0.0 | 36.4 | 0.3 ± 0.1 | 0.8 ± 0.3 | |||
| χ Cyg | 1 – a | 26.2 | –1.7 | 38.7 | 4.3 ± 1.5 | 1.7 ± 0.6 | 10.1 ± 3.6 | |
| – b | 16.2 | 1.1 | 12.4 | 3.0 ± 1.1 | 1.5 ± 0.5 | 7.5 ± 2.7 | ||
| 2 – a | 36.4 | 1.9 | 26.7 | 2.6 ± 0.3 | 2.4 ± 0.3 | |||
| – b | 50.2 | 0.0 | 33.9 | 0.9 ± 0.1 | 1.2 ± 0.1 | |||
| 3 – a | 51.8 | 0.2 | 33.9 | 1.6 ± 0.2 | 2.5 ± 0.2 | |||
| – b | 39.4 | –0.8 | 34.8 | 3.3 ± 0.3 | 2.6 ± 0.2 | |||
| 4 – a | 32.8 | –1.0 | 32.8 | 1.4 ± 0.4 | 1.4 ± 0.4 | 1.8 ± 0.5 | ||
| – b | 26.2 | –1.2 | 25.9 | 1.8 ± 0.5 | 0.7 ± 0.2 | 2.4 ± 0.7 | ||
| 5 – a | 38.9 | –1.2 | 34.0 | 2.1 ± 0.3 | 5.3 ± 0.7 | |||
| – b | 30.4 | 1.7 | 30.2 | 4.3 ± 0.6 | 1.6 ± 0.2 | 2.6 ± 0.3 | ||
| 6 – a | 28.5 | 2.2 | 28.9 | (2.3 ± 1.1) | (0.9 ± 0.4) | (1.0 ± 0.5) | * | |
| – b | 28.6 | 2.2 | 22.3 | (7.7 ± 3.5) | (3.0 ± 1.4) | (47.8 ± 22.1) | * | |
| U Her | 1 – a | 18.8 | 0.9 | 136.7 | 3.9 ± 1.8 | 1.9 ± 0.9 | 2.2 ± 1.0 | |
| (March) | – b | 1.7 | –0.4 | 93.1 | 1.6 ± 0.7 | 1.1 ± 0.5 | 11.8 ± 5.5 | |
| 2 – a | 9.4 | –0.8 | 177.9 | 1.5 ± 0.4 | 0.9 ± 0.2 | 10.5 ± 2.8 | ||
| – b | 5.0 | 0.8 | 170.6 | 1.5 ± 0.4 | 1.0 ± 0.3 | 5.9 ± 1.6 | ||
| 3 – a | 9.3 | 1.0 | 115.8 | 1.7 ± 0.8 | 1.0 ± 0.5 | 2.3 ± 1.1 | ||
| – b | 4.2 | –1.3 | 51.0 | 3.2 ± 1.5 | 2.0 ± 1.0 | 9.8 ± 4.5 | ||
| U Her | 1 – a | 13.1 | –1.2 | 162.3 | 4.4 ± 1.0 | 2.4 ± 0.6 | 4.9 ± 1.2 | |
| (May) | – b | 12.0 | 1.3 | 7.8 | 5.1 ± 1.2 | 2.8 ± 0.7 | 17.1 ± 4.0 | |
| R Leo | 1 – a | 31.2 | 2.3 | 79.2 | 6.3 ± 1.0 | 2.4 ± 0.4 | 6.9 ± 1.1 | |
| – b | 32.2 | –1.6 | 21.1 | 8.5 ± 1.3 | 3.2 ± 0.5 | 32.1 ± 5.0 | ||
| 2 – a | 10.0 | 0.7 | 15.1 | 5.7 ± 1.0 | 3.3 ± 0.6 | 8.8 ± 1.5 | ||
| – b | 8.3 | –1.2 | 152.7 | 2.1 ± 0.4 | 1.2 ± 0.2 | 2.0 ± 0.4 | ||
| 3 – a | 7.2 | –0.9 | 164.7 | 1.8 ± 0.2 | 1.1 ± 0.1 | 3.9 ± 0.4 | ||
| – b | 13.4 | 1.2 | 72.2 | 2.0 ± 0.2 | 1.1 ± 0.1 | 8.1 ± 0.8 | ||
| 4 – a | 5.5 | –0.7 | 179.7 | 0.4 ± 0.1 | 0.3 ± 0.1 | 7.6 ± 1.2 | ||
| – b | 13.4 | 1.2 | 72.2 | 0.6 ± 0.1 | 0.3 ± 0.1 | 5.2 ± 0.8 | ||
| 5 – a | 19.1 | 1.1 | 164.1 | 2.9 ± 0.2 | 1.4 ± 0.1 | 5.1 ± 0.4 | ||
| – b | 21.2 | –1.6 | 166.2 | 6.3 ± 0.5 | 2.8 ± 0.2 | 11.2 ± 0.9 | ||
| 6 – a | 16.9 | –1.8 | 171.0 | 1.7 ± 0.4 | 0.9 ± 0.2 | 6.2 ± 1.3 | ||
| – b | 16.5 | –1.6 | 173.9 | 1.8 ± 0.4 | 0.9 ± 0.2 | 13.6 ± 2.8 |
Notes. The hashtag is the number of the components described in Table 4, the two peaks for each component are represented by a and b, separated by Δv. pL, pC, and χ are the linear polarization, the circular polarization, and the angle of polarization, respectively. BE is the magnetic field value computed with Eq. (11), the second solution for pL < 33% (see Sect. 4.5.3). BZ in Col. 8 results from Eq. (15) and still depends on the angle. The asterisk in the last column indicates unreliable results.
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