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Home All issues Volume 706 (February 2026) A&A, 706 (2026) A241 Full HTML
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Table A.1

Stellar parameters of the selected sample.

D Teff log g R* M* Bp Prot†$\[P_{\mathrm{rot}}^{\dagger}\]$ LCBO
HD (pc) (kK) [cgs] (R⊙) (M⊙) (kG) (d) (erg s−1)
  11502* 53(1)[1] 10.4(0.2) 4.27−0.15+0.1$\[4.27_{-0.15}^{+0.1}\]$[4] 2.01(0.07) 2.7(0.4) 3.0−0.75+29.13$\[3.0_{-0.75}^{+29.13}\]$ n.a. n.a.
  12767 106(1) 13.4(0.2) 3.85(0.1)[5] 3.5(0.2) 4.1(0.2) 2.0−0.6+0.5$\[2.0_{-0.6}^{+0.5}\]$ 1.892(n.a.)[14] 1.11(0.69) × 1035
  15089 45.2(0.2) 8.8(0.1) 4.12−0.08+0.07$\[4.12_{-0.08}^{+0.07}\]$[4] 2.17(0.07) 2.2(0.3) 1.85−0.16+0.49$\[1.85_{-0.16}^{+0.49}\]$ 1.74050(3)[15] 1.78(0.36) × 1034
  21699 177(4) 12.5(0.2) 4.15(n.a.)[6] 4.3(0.2) 4.9(0.25) 2.8−0.1+0.5$\[2.8_{-0.1}^{+0.5}\]$ 2.49187(7)[3] 2.84(0.52) × 1035
  32633 214.5(2) 10.2(0.4) 4.224(0.063)[7] 2.9(0.2) 2.6(0.4) 17−2+1$\[17_{-2}^{+1}\]$ 6.4303(8)[16] 3.85(1.21) × 1035
  36526 415.7(8) 15(2)[3] 4.10(0.14)[8] 2.35(0.1) 4.3(0.2)[8] 11(1)[8] 1.54185(4)[17] 8.45(1.37) × 1035
  49333 216(3) 15.8(0.1)[3] 4.23(0.2)[9] 3.6(0.2) 4.5(0.2) 3.6−1.2+1$\[3.6_{-1.2}^{+1}\]$ 2.1805(1)[16] 2.95(2.02) × 1035
  49976 101.4(0.4) 9.5(0.2) 4.298(0.063)[7] 2.085(0.055) 2.4(0.3) 7.5−1.7+48.6$\[7.5_{-1.7}^{+48.6}\]$ 2.9768(2)[16] 7.98(3.65) × 1034
  55522 277(3) 16.2(0.2) 3.95(0.06)[8] 4.8(0.2) 5.2(0.3) 3.1(0.4)[8] 2.7292(3)[17] 4.67(1.42) × 1035
  62140 94.4(0.2) 7.8(0.1) 3.99(0.13)[4] 2.32(0.06) 1.9(0.3) 5.11−0.33+1.05$\[5.11_{-0.33}^{+1.05}\]$ 4.28677(3)[18] 3.25(0.52) × 1034
  65339 97(2) 8.3(0.1) 4.00(0.09)[4] 2.41(0.08) 2.0(0.3) 15.7−1.6+2.3$\[15.7_{-1.6}^{+2.3}\]$ 7.993(2)[16] 1.01(0.24) × 1035
  74067 76(1) 10.6(0.1) 4.08(0.09)[4] 2.21(0.05) 2.7(0.4) 3.44−0.07+12.2$\[3.44_{-0.07}^{+12.2}\]$ 3.115(2)[18] 1.87(0.17) × 1034
103192 95(5)[2] 11.8(0.4)[4] 3.83−0.11+0.06$\[3.83_{-0.11}^{+0.06}\]$[4] 3.9(0.4) 3.6(0.3)[4] 1.38−0.32+1.08$\[1.38_{-0.32}^{+1.08}\]$ 2.35666(2)[19] 5.56(3.11) × 1034
120198 92.8(0.3) 10.4(0.1) 4.14−0.12+0.11$\[4.14_{-0.12}^{+0.11}\]$[4] 2.235(0.055) 2.7(0.4) 1.6−0.36+0.41$\[1.6_{-0.36}^{+0.41}\]$ 1.3858(8)[20] 2.16(0.99) × 1034
122532 153.2(3) 12.8(0.3) 3.70(n.a.)[10] 2.8(0.1) 3.5(0.2) 3.0−0.9+0.7$\[3.0_{-0.9}^{+0.7}\]$ 3.6807(1)[21] 2.55(1.58) × 1034
125248 86(4) 9.7(0.1) 4.05(n.a.)[10] 1.86(0.06) 2.5(0.3) 9.0−1.1+1.3$\[9.0_{-1.1}^{+1.3}\]$ 9.302(1)[16] 6.86(1.83) × 1033
130559 75.0(0.5) 9.3(0.7) 4.07(0.10)[4] 2.1(0.2) 1.71(0.09) 2.36−0.44+0.77$\[2.36_{-0.44}^{+0.77}\]$ 1.90798(1)[18] 1.82(0.87) × 1034
133029 156.5(0.6) 12.3(0.2) 4.176(0.024)[7] 2.6(0.1) 3.5(0.2) 9.0−0.3+5.0$\[9.0_{-0.3}^{+5.0}\]$ 2.8885(2)[16] 2.58(0.45) × 1035
137909 36(1) 7.5(0.4)[4] 3.77−0.14+0.11$\[3.77_{-0.14}^{+0.11}\]$[4] 2.7(0.1) 2.6(0.1) 5.2−1+7.1$\[5.2_{-1}^{+7.1}\]$ 18.4877(15)[22] 2.87(1.19) × 1033
140160 67.8(0.3) 9.3(0.1) 4.11−0.08+0.06$\[4.11_{-0.08}^{+0.06}\]$[4] 2.18(0.06) 2.4(0.3) 1.18−0.26+0.29$\[1.18_{-0.26}^{+0.29}\]$ 1.5959(1)[18] 8.38(3.77) × 1033
140728 91.4(0.4) 10.4(0.1) 4.06−0.12+0.10$\[4.06_{-0.12}^{+0.10}\]$[4] 2.42(0.06) 2.7(0.35) 2.3−0.36+0.46$\[2.3_{-0.36}^{+0.46}\]$ 1.29559(2)[18] 7.24(2.35) × 1034
142884 173(1) 10.2(0.5) 4.344(0.063)[7] 2.82(0.09) 2.6(0.4) < 0.75 0.80296(2)[16] 4.05(0.92) × 1034
145102 178(2) 8.8(0.3) 3.83(n.a.)[11] 3.8(0.1) 2.2(0.3) < 0.98 1.4178(6)[23] 9.43(2.12) × 1034
149822 146(3) 10.4(0.2) 4.01(n.a.)[11] 2.75(0.08) 2.7(0.3) 4.0−1.1+2.1$\[4.0_{-1.1}^{+2.1}\]$ 1.966(1)[3] 1.72(0.96) × 1035
151346 194(3) 6.1(0.1) 4.27(n.a.)[11] 4.8(0.25) 2.1(0.1) < 1.7 2.180(2)[23] 3.59(0.92) × 1035
152107 53.2(0.3) 8.9(0.1) 4.06−0.06+0.05$\[4.06_{-0.06}^{+0.05}\]$[4] 2.185(0.065) 2.2(0.3) 4.2−0.20.5$\[4.2_{-0.2}^{0.5}\]$ 3.8586(6)[16] 1.89(0.26) × 1034
164224 223(3) 7.7(0.2) 4.1577(n.a.)[12] 2.27(0.08) 1.8(0.3) ≈1.7[13] 0.73(1)[24] 1.15(0.27) × 1035
168856 202(1) 8.3(0.4) 3.744(0.033)[7] 3.6(0.2) 3.15(0.2) 3.5−0.6+3.7$\[3.5_{-0.6}^{+3.7}\]$ 2.4277(1)[16] 2.80(1.06) × 1035
175132 316(4) 11.1(0.2) 3.858(0.02)[7] 5.7(0.3) 5.45(0.3) > 3.5 8.030(n.a.)[3] 1.53(0.40) × 1035
183339 320(5) 14.0(0.1) 3.87(n.a.)[11] 4.2(0.25) 4.9(0.25) > 4.5 4.204(n.a.)[3] 2.48(0.68) × 1035
224801 178(1) 12.3(0.2) 3.7(n.a.)[5] 3.0(0.15) 3.6(0.2) > 4.6 3.73980(n.a.)[25] 8.27(2.11) × 1034
345439 2330(140) 14.5(0.3) 4.29(0.19)[8] 3.7(0.5)[8] 8.3(0.8)[8] 8.9(1.1)[8] 0.77018(2)[26] 1.19(0.59) × 1037

Notes: * For the star HD 11502, we made a mistake when the present project was planned; we wrongly assumed the stellar rotation period of the close star HD 11503 (separation about 7.5 arcsec). The following critical analysis of each target revealed our mistake; therefore, we cannot calculate the value of the LCBO of HD 11502. † The uncertainty in the least significant digit is reported in parentheses.

References: The distances of almost all sources are the median of the photogeometric distance posterior given by Bailer-Jones et al. (2021). The effective temperatures, stellar radii, and masses are mainly taken from the TESS Input Catalog v8.0 (Stassun et al. 2019) and v8.2 (Paegert et al. 2021), and from Kervella et al. (2022), whereas the polar magnetic field strength is from Sikora et al. (2019a) and Shultz et al. (2022). [1] Bailer-Jones et al. (2018); [2] van Leeuwen (2007); [3] Shultz et al. (2022); [4] Sikora et al. (2019a); [5] Soubiran et al. (2016); [6] Glagolevskij et al. (2006); [7] Abdurro’uf et al. (2022); [8] Shultz et al. (2019); [9] Cidale et al. (2007); [10] Ghazaryan et al. (2018); [11] Glagolevskij (2019); [12] Fouesneau et al. (2022); [13] Bowman et al. (2018); [14] Renson & Catalano (2001); [15] Musielok et al. (1980); [16] Bernhard et al. (2020); [17] Shultz et al. (2018); [18] Sikora et al. (2019b); [19] Manfroid & Renson (1994); [20] Wade et al. (1998); [21] Lanz & Mathys (1991); [22] Bagnulo et al. (1999); [23] Wraight et al. (2012); [24] Buysschaert et al. (2018); [25] Catalano & Renson (1998). [26] Hubrig et al. (2017).

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