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Table 4

Theoretical quantities derived from the evolution models for the Zeeman detected giants.

HD Name M ∗ Evolution R BCE τ(Hp/ 2) R (Hp/ 2) τ(max) R max τ(RCE/ 2) R (RCE/ 2)
M ⊙ phase R ∗ day R ∗ day R ∗ day R ∗
Active Giants
3229 14 Cet 1.55 ± 0.1 HGap 0.936 0.68 0.94 1.52 0.94 0.27 0.97
4128 β Cet 3.5 ± 0.2 He burning 0.504 121 0.56 232 0.51 53 0.75
3.6 ± 0.2 Base RGB 0.47 135 0.53 246 0.48 59 0.73
9746 OP And 2.0 ± 0.5 RGB (Li) 0.044 25 0.06 160 0.79 118 0.52
2.0 ± 0.5 He burning 0.183 106 0.23 179 0.45 80 0.60
27536 EK Eri 1.9 ± 0.3 Base RGB 0.507 103 0.56 234 0.51 43 0.75
28307 77 Tau 3. ± 0.2 Base RGB 0.553 95 0.62 179 0.57 41 0.79
31993 V1192 Ori 1.8 ± 0.5 RGB (Li) 0.054 32 0.07 129 0.36 107 0.53
1.7 ± 0.5 He burning 0.244 99 0.32 190 0.27 62 0.68
2. ± 0.5 RGB 0.059 37 0.08 145 0.34 116 0.53
33798 V390 Aur 2.25(*) ± 0.3 Base RGB 0.477 119 0.56 230 0.50 49 0.77
47442 ν3 CMa 4.5 ± 0.5 Base RGB 0.415 170 0.48 314 0.43 78 0.71
4.0 ± 0.5 He burning 0.401 160 0.46 300 0.41 74 0.71
68290 19 Pup 2.5 ± 0.2 Base RGB 0.483 118 0.57 239 0.51 49 0.77
2.5 ± 0.2 He burning 0.406 162 0.47 335 0.41 67 0.71
72146 FI Cnc 2.4 ± 0.3 Base RGB 0.608 65 0.68 122 0.63 28 0.82
82210 24 UMa 1.9 ± 0.1 Base RGB 0.625 55 0.67 95 0.63 24 0.81
85444 39 Hya 3.75(*) ± 0.2 BaseRGB 0.639 59 0.69 101 0.65 26 0.83
111812 31 Com 2.75(*) ± 0.1 HGap 0.745 34 0.75 58 0.74 15 0.85
112989 37 Com 5.25 ± 0.4 He burning 0.977 91 61 154 0.57 38 0.78
5.25 ± 0.4 Base RGB 0.527 124 0.58 224 0.53 54 0.76
121107 7 Boo 4.0 ± 0.7 HGap 0.729 34 0.75 63 0.72 14 0.86
141714 δ CrB 2.5 ± 0.1 Base RGB 0.457 133 0.52 271 0.47 56 0.74
145001 κ HerA 3.5 ± 0.3 Base RGB 0.654 50 0.71 85 0.66 22 0.83
150997 η Her 2.5 ± 0.3 Base RBG 0.512 110 0.58 217 0.53 47 0.77
2.7(*) ± 0.3 He burning 0.456 126 0.52 244 0.46 54 0.73
163993 ξ Her 3. ± 0.3 Base RGB 0.570 87 0.63 161 0.58 37 0.80
2.5 ± 0.3 He burning 0.451 119 0.52 209 0.47 51 0.73
203387 ι Cap 3. ± 0.2 Base RGB 0.663 48 0.71 79 0.67 21 0.84
205435 ρ Cyg 2.6 ± 0.2 Base RGB 0.449 141 0.51 289 0.45 59 0.73
218153 KU Peg 2.5 ± 0.2 Base RGB 0.562 85 0.65 165 0.60 36 0.82
223460 OU And 2.8 ± 0.2 HGap 0.755 15 0.83 36 0.76 9 0.88
CFHT and miscellaneous
9270 η Psc 4.9 ± 0.5 Base RGB 0.640 67 0.68 121 0.644 28 0.820
28305 ϵ Tau 3.0 ± 0.2 Base RGB 0.387 168 0.45 335 0.39 73 0.69
2.5 ± 0.2 He burning 0.360 146 0.43 268 0.37 67 0.69
29139 Aldebaran 1.7 ± 0.5 AGB 0.048 31 0.06 284 0.98 104 0.53
2.0 ± 0.5 RGB 0.061 40 0.08 143 0.35 114 0.54
62509 Pollux 2.5 ± 0.3 Base RGB 0.382 162 0.45 330 0.39 68 0.68
2.5 ± 0.3 He burning 0.366 183 0.43 391 0.36 75 0.68
81797 Alphard 3.5 ± 0.5 AGB 0.064 59 0.07 768 0.93 142 0.49
124897 Arcturus 1.5(a)± 0.3 AGB 0.095 50 0.12 170 0.98 72 0.55
1.5(a)± 0.3 RGB 0.034 151 0.04 137 0.95 94 0.52

Notes. For each star we give: stellar mass, evolution phase, radius at the base of the convective envelope, and convective turnover times at different locations within the convective envelope. M∗ marked (*) indicates that the values are the result of the linear interpolation between two models. For some stars we indicate two possible evolution states (“RGB(Li)” means that we use the Li abundance as an additional indicator). The mass of Arcturus(a) is determined based on models computed at the metallicity of this star ([Fe/H] = −0.6; Lagarde et al. 2012).

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