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Table 2

Sample of stars used for this study’s statistical analysis.

Name Age (Myr) Mass (M⊙) Sp. type
HIP 58452 20−5+5$\[20_{-5}^{+5}\]$ 3.0 ± 0.3 B8.5V
HIP 58901 13−3+3$\[13_{-3}^{+3}\]$ 2.9 ± 0.3 B9V
HIP 60009 12−2+4$\[12_{-2}^{+4}\]$ 6.5 ± 0.6 B2.5V
HIP 60379 13−3+3$\[13_{-3}^{+3}\]$ 3.8 ± 0.4 B7V
HIP 60823(*1) 17−3+3$\[17_{-3}^{+3}\]$ 7.2 ± 0.7 B2V
HIP 61585(*1) 15−3+3$\[15_{-3}^{+3}\]$ 9.8−1.0+1.1$\[9.8_{-1.0}^{+1.1}\]$ B2V
HIP 62058 15−3+3$\[15_{-3}^{+3}\]$ 3.4 ± 0.3 B
HIP 62327(*1) 17−3+3$\[17_{-3}^{+3}\]$ 5.4 ± 0.5 B2.5V
HIP 63003 16−3+3$\[16_{-3}^{+3}\]$ 7.1 ± 0.7 B2V
HIP 65112 15−3+3$\[15_{-3}^{+3}\]$ 4.0 ± 0.4 B5V
HIP 66454 17−3+3$\[17_{-3}^{+3}\]$ 4.0 ± 0.4 B8V
HIP 67464(*1) 18−5+3$\[18_{-5}^{+3}\]$ 8.2 ± 0.8 B2V
HIP 67669(*1) 17−3+3$\[17_{-3}^{+3}\]$ 4.8 ± 0.5 B5V
HIP 67703 16−3+3$\[16_{-3}^{+3}\]$ 3.4 ± 0.3 B8V
HIP 68245 17−3+3$\[17_{-3}^{+3}\]$ 7.9 ± 0.8 B2V
HIP 68282(*1) 21−2+4$\[21_{-2}^{+4}\]$ 6.6 ± 0.7 B2V
HIP 69011 17−3+3$\[17_{-3}^{+3}\]$ 2.3 ± 0.2 B9.5V
HIP 70300 17−5+3$\[17_{-5}^{+3}\]$ 5.9 ± 0.6 B2V
HIP 70626 15−3+3$\[15_{-3}^{+3}\]$ 3.3 ± 0.3 B9V
HIP 71352 15−3+3$\[15_{-3}^{+3}\]$ 9.7 ± 1.0 B2V
HIP 71536(*2) 14−4+4$\[14_{-4}^{+4}\]$ 6.2 ± 0.6 B3.5V
HIP 71865(*2) 14−3+3$\[14_{-3}^{+3}\]$ 5.9 ± 0.6 B2.5V
HIP 74950(*1) 18−3+3$\[18_{-3}^{+3}\]$ 4.4 ± 0.4 B7V
HIP 76591 17−3+3$\[17_{-3}^{+3}\]$ 3.0 ± 0.3 B9V
HIP 76600(*1) 13−3+4$\[13_{-3}^{+4}\]$ 7.5 ± 0.7 B2.5V
HIP 76633 7−2+3$\[7_{-2}^{+3}\]$ 2.4 ± 0.2 B9V
HIP 77562 17−3+3$\[17_{-3}^{+3}\]$ 2.9 ± 0.3 B9V
HIP 77968 17−2+5$\[17_{-2}^{+5}\]$ 3.4 ± 0.3 B8V
HIP 78207 0.5−0.2+0.5$\[0.5_{-0.2}^{+0.5}\]$ 4.7 ± 0.5 B5V
HIP 79044(*1) 17−3+3$\[17_{-3}^{+3}\]$ 2.7 ± 0.3 B9V
HIP 80911 16−4+4$\[16_{-4}^{+4}\]$ 8.8 ± 0.9 B2V
HIP 82514(*1) 20−4+4$\[20_{-4}^{+4}\]$ 10.0 ± 1.0 B1V
HIP 82545 20−4+4$\[20_{-4}^{+4}\]$ 9.1 ± 0.3 B2V

Notes. (*)Star is a short separation (<0.1″) binary. Binarity source:(*1), from Gratton et al. (2023);(*2), from Rizzuto et al. (2013). Spectral types are from Simbad.

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