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Table 2b:

Same as for Table 2a, but now for some well-studied SPBs.

HD
Alternative Spectral $T_{\rm eff}$  $\log g$  n(He)/n(H) $\hbox{$\log~n$ (Si)/$n$ (H)}$ $\xi $ $\nu \sin i$ $\nu _{\rm macro}$
number name Type (K) (cgs)     (km s-1) (km s-1) (km s-1)
3360 $\zeta$ Cas B2IV 22000 3.80 0.10 -4.76 <3 18 $\pm$2 13
    a 22000 3.70   -4.72 $\pm$ 0.30 1 $\pm$ 1 19 $\pm$ 1 -
85953 V335 Vel B2IV 20000 3.80 0.10 -4.84 6 30 $\pm$1 20
    a 21000 3.80   -4.75 $\pm$ 0.30 1 $\pm$ 1 29 $\pm$ 2 -
3379 53 Psc B2.5IV 20000 4.30 0.10 -4.73 <3 48 $\pm$8 43
74195 o Vel B3IV 16500 3.70 0.10 -4.79 <3 18 $\pm$ 2 18
160762 $\iota$ Her B3IV 19500 4.10 0.10 -4.86 3 8$\pm$2 0
25558 40 Tau B3V 17500 4.00 0.10 -4.72 6 28 $\pm$ 2 31
181558 HR 7339 B5III 15000 4.00 0.10 -4.79 6 17 $\pm$2 0
26326 HR 1288 B5IV 15500 3.60 0.10 -4.49 <3 17 $\pm$1 17
206540 HR 8292 B5IV 13500 3.80 0.10 -4.79 3 15 $\pm$ 2 0
24587 HR 1213 B5V 14500 4.00 0.10 -4.79 <3 25 $\pm$4 21
28114 HR 1397 B6IV 14000 3.50 0.10 -4.79 <3 21 $\pm$4 17
138764 HR 5780 B6IV 14500 3.90 0.10 -4.51 3 21 $\pm$ 2 0
215573 HR 8663 B6IV 13500 3.80 0.10 -4.49 <3 8 $\pm$1 0
39844 HR 2064 B6V 14500 3.70 0.10 -4.39 <3 16 $\pm$1 0
191295 V1473 Aql B7III 13000 3.70 0.10 -4.79 3 16 $\pm$1 15
21071 V576 Per B7V 13500 3.70 0.10 -4.79 3 22 $\pm$ 1 0
37151 V1179 Ori B8V 12500 3.80 0.10 -4.79 <3 20 $\pm$2 0

Notes. (a) Independent results of the DETAIL/SURFACE analysis by Briquet & Morel (2007).


Source LaTeX | All tables | In the text

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