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Table 2a:

Fundamental parameters of well-studied $\beta $Cephei stars (spectral types from SIMBAD), as derived from AnalyseBstar (values from the closest grid model are listed).

HD
Alternative Spectral $T_{\rm eff}$  $\log g$a n(He)/n(H)b $\hbox{$\log~n$ (Si)/$n$ (H)}$ c $\xi $ $\nu \sin i$ $\nu _{\rm macro}$
number name type (K) (cgs)     (km s-1) (km s-1) (km s-1)
46328 $\xi^1$ CMa B0.5-B1IV 27000 3.80 0.10 -4.69 6 9 $\pm$ 2 11
      27500 3.75   -4.87 $\pm$0.21 6 $\pm$ 2 $10 \pm 2$ -
50707 15 CMa B1III 24000 3.40 0.10 -4.79 12 34 $\pm$ 4 38
      26000 3.60   -4.69 $\pm$0.30 7 $\pm$ 3 $45 \pm 3$ -
205 021 $\beta $ Cep B1IV 25000 3.80 0.10 -4.70 6 26 $\pm$3 24
      26000 3.70   -4.89 $\pm$0.23 6 $\pm$ 3 29 $\pm$ 2 -
44743 $\beta $ CMa B1.5III 24000 3.50 0.10 -4.76 15 19 $\pm$4 20
      24 000 3.50   -4.83 $\pm$0.23 14 $\pm$3 23 $\pm$ 2 -
214 993 12 Lac B1.5IV 23000 3.60 0.10 -4.41 6 44 $\pm$6 37
            [-4.83] [12]   [0] (forced)
      24500 3.65   -4.89 $\pm$0.27 10 $\pm$ 4 42 $\pm$ 4 -
16582 $\delta$ Ceti B1.5-B2IV 23000 3.90 0.10 -4.80 6 14 $\pm$ 2 0
      23000 3.80   -4.72 $\pm$0.29 1 +3-1 14 $\pm$ 1 -
886 $\gamma$ Peg B1.5-B2IV 23000 3.80 0.10 -4.84 <3 10 $\pm$ 1 0
      22500 3.75   -4.81 $\pm$0.29 1 +2-1 10 $\pm$ 1 -
29248 $\nu$ Eri B1.5-B2IV 23000 3.70 0.10 -4.73 10 21 $\pm$3 39
      23500 3.75   -4.79 $\pm$0.26 10 $\pm$ 4 36 $\pm$ 3 -

Notes. In italics, we display the results from the DETAIL/SURFACE analysis by Morel et al. (2006,2008). (a) Not corrected for centrifugal acceleration due to stellar rotation. (b) Solar helium abundance: n(He)/n(H) = 0.10. (c) Solar silicon abundance: $\hbox{$\log~n$ (Si)/$n$ (H)}= -4.49$. Interpolated values are listed.


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