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Table 2
Effective temperatures as derived based on angular diameter measurements (Mozurkewich et al. 2003) listed for the nine giants in our sample.
HIP | Name | Teff,ref | Teff | log g | [Fe/H] |
|
|||||
HIP 9884 | α Ari | 4493 ± 55 | 4464 | 2.27 | –0.24 |
HIP 46390 | α Hya | 4060 ± 50 | 4095 | 1.56 | –0.10 |
HIP 54539 | ψ UMa | 4550 ± 56 | 4534 | 2.33 | –0.10 |
HIP 55219 | ν UMa | 4091 ± 50 | 4133 | 1.65 | –0.17 |
HIP 72607 | β UMi | 3849 ± 47 | 3992 | 1.32 | –0.23 |
HIP 74666 | δ Boo | 4850 ± 60 | 4861 | 2.63 | –0.37 |
HIP 77070 | α Ser | 4558 ± 56 | 4540 | 2.61 | 0.16 |
HIP 94376 | δ Dra | 4851 ± 67 | 4807 | 2.71 | –0.17 |
HIP 102488 | ϵ Cyg | 4756 ± 59 | 4711 | 2.59 | –0.18 |
Notes. Also listed are the stellar parameters determined using our analysis based on observations from a FIES, NARVAL, or ESpaDOnS spectrum for the corresponding star.
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