Table 1.
Stellar parameters for the stars employed in this study, including previously obtained average large-scale magnetic field strength from Stokes V, if available.
Star | Teff (K) | log g (cms−2) | εFe | v sin i (kms−1) | ⟨B⟩V (G) | References |
---|---|---|---|---|---|---|
HD 1835 | 5837 | 4.47 | −4.29 | 6.3 | 19 | 1, 2 |
HD 3651 | 5284 | 4.53 | −4.38 | 1.1 | 3.58 | 3, 4 |
HD 9986 | 5805 | 4.45 | −4.46 | 2.6 | 0.605 | 1, 4 |
HD 10476 | 5181 | 4.54 | −4.58 | 0.1 | 3.3 | 1, 5 |
HD 20630 | 5742 | 4.49 | −4.42 | 4.7 | 26.3 | 1, 4 |
HD 22049 | 5146 | 4.57 | −4.57 | 2.4 | 10 – 20 | 1, 6, 7 |
HD 59967 | 5848 | 4.54 | −4.57 | 4.0 | – | 8, 9 |
HD 73256 | 5532 | 4.49 | −4.28 | 3.2 | 2.7 | 3, 10 |
HD 73350 | 5802 | 4.48 | −4.42 | 3.2 | 11 | 1, 4 |
HD 75732 | 5235 | 4.45 | −4.23 | 2.5 | 3.4 | 1, 11 |
HD 76151 | 5790 | 4.55 | −4.43 | 0.0 | 2.99 | 1, 4 |
HD 102195 | 5330 | 4.37 | −4.44 | 2.9 | 10.7 | 10,12 |
HD 130322 | 5308 | 4.41 | −4.53 | 1.6 | 2.34 | 1,10 |
HD 131156 A | 5570 | 4.65 | −4.58 | 4.9 | 22.2 – 61.8 | 1, 4 |
HD 179949 | 6168 | 4.34 | −4.40 | 7.0 | 2.6 – 3.7 | 10 |
HD 206860 | 5974 | 4.47 | −4.56 | 10.1 | 11 – 24 | 1, 2 |
Notes. 1: Valenti & Fischer (2005), 2: Rosén et al. (2016), 3: Bonfanti et al. (2015), 4: See et al. (2019), 5: Marsden et al. (2014), 6: Jeffers et al. (2014), 7: Petit et al. (2021), 8: Yana Galarza et al. (2019), 9: Lorenzo-Oliveira et al. (2019), 10: Fares et al. (2013), 11: Folsom & Fionnagáin (2020), 12: Ge et al. (2006). Fe abundance is defined as log(NFe/Ntotal).
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