Table 2: Median values for the macroturbulent ( v$_{\rm m}$) and projected rotational ( v sin  i) velocities deduced for the SMC datasets presented in Dufton et al. (2005) and by Trundle et al. (2004). Also listed are estimates for the Galactic supergiants discussed by Ryans et al. (2002). The sources of the spectral types and effective temperatures are discussed in the text.
Star Spectral $T_{\rm eff}$ Dataset v sin  i v$_{\rm m}$
  type K   km s-1
SMC          
AzV 487 BC0Ia 27 000 AAT 50 54
AzV 215 BN0Ia 26 750 AAT/VLT 66 55
AzV 242 B1Ia 21 500 AAT 54 43
AzV 78 B1.5Ia+ 21 250 AAT 46 36
Sk 191 B1.5Ia 21 500 VLT/AAT 92 49
AzV 210 B1.5Ia 20 500 VLT 37 36
AzV 462 B1.5Ia 19 000 AAT 43 26
AzV 303 B1.5Iab 18 000 AAT 42 26
AzV 472 B2Ia 19 000 AAT 33 27
AzV 18 B2Ia 19 000 VLT 33 30
AzV 374 B2Ib 18 500 AAT 47 20
AzV 362 B3Ia 14 000 VLT 38 30
AzV 22 B5Ia 14 500 VLT 33 23
Galactic          
HD 204172 B0.2 Ia 28 500 WHT 62 62
HD 38771 B0.5 Ia 27 500 McDonald 50 55
HD 2905 BC0.7 Ia 24 000 McDonald 52 59
HD 13854 B1 Iab 23 500 McDonald 32 53
HD 24398 B1 Ib 23 000 McDonald 36 38
HD 193183 B1.5 Ib 22 500 WHT 45 40
HD 41117 B2 Ia 19 500 McDonald 41 38
HD 206165 B2 Ib 20 000 WHT 35 34
HD 34085 B8 Ia 13 000 McDonald 25 28
HD 208501 B8 Ib 13 000 WHT 28 27
HD 21291 B9 Ia 11 500 McDonald 17 21


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