Table 1
Sample of stars.
| HD number | Other Id. | Sp. Tp. | B-V | Prot[Pmin – Pmax] | Pcyc | ![]() |
|---|---|---|---|---|---|---|
| (days) | (years) | |||||
| Sun | G2 V | 0.66 | 25.4 [24.5–28.5] | 10.9 | −4.901 | |
| Prot < 30 days | ||||||
| HD 1835 | BE Cet | G2.5 V | 0.66 | 7.78 [7.23–8.30] | 9.1 | −4.433 |
| HD 20630 | κ Cet | G5 V | 0.68 | 9.24 [9.01–9.48] | 5.6 | −4.420 |
| HD 76151 | HIP 43726 | G3 V | 0.67 | 15 | 2.52 | −4.659 |
| HD 78366 | HIP 44897 | G0 V | 0.60 | 9.67 [9.12–10.19] | 12.2 – 5.9 | −4.608 |
| HD 100180 | 88 Leo | F7 V | 0.57 | 14 | 3.6–12.9 | −4.922 |
| HD 114710 | β Com | F9.5 V | 0.58 | 12.35 [11.43–13.54] | 16.6 – 9.6 | −4.745 |
| HD 115404 | HIP 64797 | K1 V | 0.94 | 18.47 [17.24–19.90] | 12.4 | −4.480 |
| HD 149661 | 12 Oph | K2 V | 0.84 | 21.07 [20.6–22.9] | 16.2–4 | −4.583 |
| HD 152391 | HIP 82588 | G7 V | 0.76 | 11.43 [10.20–12.97] | 10.9 | −4.448 |
| HD 156026 | HIP 84478 | K5 V | 1.16 | 21 | 21.0 | −4.662 |
| HD 165341 A | 70 Oph A | K1 V | 0.86 | 19.9 | 15.5–5.1 | −4.548 |
| HD 190406 | 15 Sge | G1 V | 0.61 | 13.94[12.67–15.57] | 2.6–16.9 | −4.797 |
| Prot > 30 days | ||||||
| HD 3651 | 54Psc | K0 V | 0.85 | 44 | 14.6 | –4.991 |
| HD 4628 | HIP 3765 | K2 V | 0.88 | 38.5 [37.2–41.4] | 8.6 | −4.852 |
| HD 10476 | HIP 7981 | K1 V | 0.84 | 35.2 [34.0–37.3] | 9.6 | −4.912 |
| HD 16160 | HIP 12114 | K3 V | 0.98 | 48.0 [42.2–51.5] | 13.2 | −4.958 |
| HD 26965 | 40 Eri | K1 V | 0.82 | 43 | 10.1 | −4.872 |
| HD 32147 | HIP 23311 | K5 V | 1.06 | 48.0 | 11.1 | −4.948 |
| HD 81809 | HIP 46404 | K0 V | 0.80 | 40.2[37.0–43.0] | 8.2 | −4.921 |
| HD 103095 | HIP 57939 | G8 V | 0.75 | 31 | 7.3 | −4.896 |
| HD 160346 | HIP 86400 | K3 V | 0.96 | 36.4 [35.4–37.8] | 7.0 | −4.795 |
| HD 166620 | HIP 88972 | K2 V | 0.87 | 42.4 [33.4–50.8] | 15.8 | −4.955 |
| HD 201091 | 61 Cyg A | K5 V | 1.17 | 35.37 [26.82–45.25] | 7.3 | −4.764 |
| HD 201092 | 61 Cyg B | K7 V | 1.37 | 37.84 [31.78–46.57] | 10.5 | −4.764 |
| HD 219834B | 94 Aqr B | K2 V | 0.91 | 43 | 10.0 | −4.944 |
Notes. All parameters are taken from Saar & Brandenburg (1999) and Paper I. The range in Prot has been taken from Donahue et al. (1996). Column 5 shows the cycle periods; in case there are double periodicities, they appear in the same order than in Saar & Brandenburg (1999), i.e. the primary before the secondary.
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