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Table 1:

Si IV SEI model profile fitting parameters for the core sample.

Star 		Sp. type $T_{\rm eff}$ (kK) $v_\infty $ $\beta$ $v_{\rm turb}$ $\tau_{{\rm rad}}(w)$(blue/red) $\langle$$\dot M$ qi$\rangle$(blue) $\langle$$\dot M$ qi$\rangle$(red)
              (10 $^{-9}~M_\odot$ yr-1) (10 $^{-9}~M_\odot$ yr-1)
HD 13866 B2 Ib-II:p 18.8 860 0.7 0.03 1.45 0.52 0.70
HD 14134 B3 Ia 16.5 495 0.5 0.10 1.37 0.83 1.39
HD 14143 B2 Ia 18.0 525 3.5 0.25 1.80 7.46 8.36
HD 36371 B4 Ib 16.5 465 0.8 0.17 1.10 0.38 0.46
HD 42087 B2.5 Ib 18.0 630 1.2 0.11 1.04 0.66 1.24
HD 43384 B3 Iab 16.5 630 0.9 0.20 1.19 1.11 2.82
HD 47240 B1 Ib 20.5 955 1.0 0.07 1.04 1.36 2.99
HD 51309 B3 Ib 16.5 730 0.5 0.15 1.55 0.94 1.81
HD 53138 B3 Ia 16.5 515 1.1 0.28 1.22 1.97 2.28
HD 58350 B5 Ia 15.0 380 0.8 0.25 2.04 0.90 1.25
HD 58510 B1 Ib-II 20.5 915 0.9 0.19 1.79 1.37 1.62
HD 77581 B0.5 Iae 26.0 655 1.0 0.22 1.80 1.19 1.72
HD 79186 B5 Ia 15.0 435 0.8 0.23 1.73 0.86 1.09
HD 93827 B1 Ib 20.5 590 0.5 0.16 1.64 0.10 0.15
HD 111934 B1.5 Ib 18.5 935 3.1 0.15 1.46 4.62 6.35
HD 111973 B3 Ia 16.5 520 0.5 0.25 1.43 0.87 1.31
HD 111990 B2 Ib 18.0 715 3.3 0.12 1.97 2.14 2.50
HD 119608 B1 Ib 20.5 925 0.6 0.25 1.14 2.05 3.69
HD 148379 B2 Iap 18.0 560 3.2 0.17 1.32 3.78 9.86
HD 152236 B0.5 Ia 26.0 470 2.0 0.31 1.12 1.42 2.03
HD 152667 B0 Ia 27.5 800 2.5 0.28 1.78 4.44 4.81
HD 155985 B0.7 Ib 23.5 940 0.5 0.13 1.24 0.60 0.95
HD 157246 B1 Ib 20.5 600 0.5 0.31 1.08 0.67 1.56
HD 198478 B2.5 Ia 17.5 560 2.0 0.24 1.34 2.14 4.16
HD 225094 B3 Ia 16.5 485 0.5 0.21 1.75 0.81 0.78

Notes.  $T_{\rm eff}$ from Searle et al. (2008). The $\langle$$\dot M$ qi$\rangle$ values include a few cases where  $\tau_{{\rm rad}}(w)$ exceeds 5.0 in isolated velocity bins.


Source LaTeX | All tables | In the text

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