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Table 5
Comparison of results from Shultz et al. (2019) and this work.
| Parameter | HD 37061 Aa | HD 37061 Ab | HD 37061 C |
|---|---|---|---|
| Teff (kK) | 30.5(5) | 15.2(14) | 22.2(10) |
| 31.1(5) | 15.7(5) | 22.3(5) | |
| log 𝑔 | 4.2(1) | 4.33(1) | 4.28(2) |
| 4.15(5) | 4.28(10) | 4.25(10) | |
| Mevol (M⊙) | 14.9(5) | 3.9(7) | 7.8(7) |
| 16.4(4) | 4.4(2) | 8.1(4) | |
| R(R⊙) | 5.1(3) | 2.2(2) | 3.3(2) |
| 5.7(3) | 2.5(3) | 3.6(4) | |
| log L/L⊙ | 4.29(9) | 2.4(3) | 3.3(2) |
| 4.43(4) | 2.54(8) | 3.45(8) | |
| v sin i (km s−1) | 190(10) | 10(5) | 100(10) |
| 190(10) | 8(3) | 104(10) | |
| irot (º) | … | … | 38(5) |
| … | … | 39(7) | |
| a (AU) | … | … | 3.38(26) |
| … | … | 3.77(12) |
Notes. In each doublet of values, the upper one is from Shultz et al. (2019) and the lower is from the present work. We adopted the rotational period and angular separation of HD 37061 C from Shultz et al. (2019). To calculate a, we used the Gaia DR3 distance.
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