Table 4: Four stars from Table 3 with photometric distances and reddenings consistent with the SWB around 3C 434.1. Sources of the physical values $v_{\infty }$, luminosity, mass and effective temperature are from Schaerer & de Koter (1997).
Star Type $\alpha $,$\delta $ $v_{\infty }$ log( $L/L_{\odot }$) M $T_{\rm eff}$ $\dot{M}$/10-6 $L_{\rm w}$/1036 $\dot{M}_{6}v_{2000}^{2}$
  (range) (J2000) (km s-1)   ( $M_{\odot}$) (K) ( $M_{\odot}$ yr-1) (erg s-1)  
1 B0 21$^{\rm h}$25$^{\rm m}$46.2$^{\rm s}$ 2890 4.658 20 35 500 0.088 0.23 0.18
  (O9-B1) 51 $\hbox{$^\circ$ }$54$^\prime$52.5 $^{\prime\prime}$              
4 B0 21$^{\rm h}$25$^{\rm m}$18.7$^{\rm s}$ 2890 4.658 20 35 500 0.088 0.23 0.18
  (O9-B1) 51 $\hbox{$^\circ$ }$57$^\prime$29.2 $^{\prime\prime}$              
7 O4 21$^{\rm h}$24$^{\rm m}$33.7$^{\rm s}$ 3100 5.85 70 50 000 1.30 3.94 3.12
  (O3-O5) 51 $\hbox{$^\circ$ }$59$^\prime$19.4$^\prime$              
10 B0 21$^{\rm h}$25$^{\rm m}$28.8$^{\rm s}$ 2890 4.658 20 35 500 0.088 0.23 0.18
  (O9-B1) 51 $\hbox{$^\circ$ }$54$^\prime$59.3 $^{\prime\prime}$              


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