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Table 4

Best-fit Zeeman broadening results for ϵ Eridani.

Two-component model
Parameter 21 September 22 September 24 September 25 September Average
Teff (K) 5010
log g (cgs) 4.53
v sin i (km s−1) 2.59
ξmic (km s−1) 0.99
ξmac (km s−1) 4.93 ± 0.24 3.03 ± 0.24 3.34 ± 0.18 3.19 ± 0.22 3.26 ± 0.17
Metallicity 0.038 ± 0.007 0.024 ± 0.010 0.015 ± 0.008 0.012 ± 0.009 0.022 ± 0.010
Bmono (G) 1898 ± 129 1812 ± 136 1846 ± 133 1783 ± 135 1835 ± 43
Filling factor 0.125 ± 0.017 0.159 ± 0.023 0.126 ± 0.018 0.141 ± 0.021 0.138 ± 0.014

Multi-component model
Parameter 21 September 22 September 24 September 25 September Average

Teff (K) 5010
log g (cgs) 4.53
v sin i (km s−1) 2.59
ξmic (km s−1) 0.99
ξmac (km s−1) 5.02 ± 0.21 3.22 ± 0.19 3.44 ± 0.19 3.40 ± 0.18 3.40 ± 0.12
Metallicity 0.048 ± 0.012 0.029 ± 0.016 − 0.008 ± 0.015 0.005 ± 0.014 0.019 ± 0.022
f0 kG 0.831 ± 0.043 0.840 ± 0.057 0.850 ± 0.054 0.859 ± 0.051 0.845 ± 0.011
f2 kG 0.118 ± 0.017 0.131 ± 0.023 0.140 ± 0.022 0.129 ± 0.020 0.130 ± 0.008
f4 kG 0.000 ± 0.022 0.028 ± 0.028 0.009 ± 0.026 0.010 ± 0.025 0.012 ± 0.010
f6 kG 0.050 ± 0.033 0.000 ± 0.044 0.000 ± 0.042 0.000 ± 0.040 0.013 ± 0.021

Notes. The results are presented for the two-component model and for a multi-component model that provides limits on the presence of stronger magnetic fields. The parameters without uncertainties were fixed based on a fit to the visible spectrum. The final column contains averages over the four nights, where the standard deviation is used as the uncertainty.

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