Table 2: OVI column density summary.
      OVI(1032 Å)       OI(1039 Å)   CII(1036 Å)  
star SNR $W_{\lambda}$(OVI) $V_{\odot}$ $\it b$ log N(OVI) $n_{\rm OVI}$ $W_{\lambda}$(OI) $V_{\odot}$ $W_{\lambda}$(CII) $V_{\odot}$
    (mÅ) (km s-1) (km s-1) (cm-2) (cm-3) (mÅ) (km s-1) (mÅ) (km s-1)
HD 560 9:1 <13.7 - - <13.04 <3.5 $\times $ 10-8 76.5 $\pm$ 10 -21.5 90.5 $\pm$ 13 -20.0
HD 20863 9:1 30.0 $\pm$ 9.5 +6.0 13.5 $\pm$ 4 13.48 $\pm$ 0.09 5.8 $\times $ 10-8 110.0 $\pm$ 30 +4.0 98.5 $\pm$ 20 +4.0
HD 26670 7:1 <17.5 - - <13.15 <3.7 $\times $ 10-8 74.5 $\pm$ 8 +6.0 107 $\pm$ 35 +12.5
HD 74604 17:1 11.5 $\pm$ 4.0 -4.4 13.6 $\pm$ 5 12.98 $\pm$ 0.15 2.0 $\times $ 10-8 60.0 $\pm$ 10 -15.0 85 $\pm$ 10 -9.0
HD 75311 14:1 <10.5 - - <12.93 <1.6 $\times $ 10-8 90.0 $\pm$ 9 +13.1 115 $\pm$ 15 +14.5
HD 75416 10:1 <12.7 - - <13.00 <3.3 $\times $ 10-8 78.0 $\pm$ 9 +11.0 115 $\pm$ 20 +11.5
HD 90972 10:1 <10.6 - - <12.92 <1.8 $\times $ 10-8 55.0 $\pm$ 8 +12.0 86 $\pm$ 14 +4.5
HD 110020 7:1 <16.8 - - <13.13 <4.0 $\times $ 10-8 65.0 $\pm$ 8 +4.5 89 $\pm$ 17 +2.0
HD 124367 18:1 27.5 $\pm$ 8.5 -5.8 14.6 $\pm$ 4 13.39 $\pm$ 0.13 5.3 $\times $ 10-8 105 $\pm$ 10 -2.0 175 $\pm$ 27 +4.0
HD 139006 10:1 <15.5 - - <13.09 < 1.7 $\times $ 10-7 15.5 $\pm$ 5 -18.0 61 $\pm$ 9 -16.0
HD 148594 7:1 <14.0 - - <13.05 < 2.2 $\times $ 10-8 145 $\pm$ 15 -7.5 N/A* -
HD 149630 14:1 22.0 $\pm$ 7.0 +16.9 19.1 $\pm$ 6 13.32 $\pm$ 0.23 7.3 $\times $ 10-8 45.0 $\pm$ 8 -11.0 150 $\pm$ 11 -12.0
HD 149730 13:1 17.5 $\pm$ 6.0 -11.2 20.8 $\pm$ 6 13.16 $\pm$ 0.13 5.8 $\times $ 10-8 115.0 $\pm$ 12 0.0 180 $\pm$ 20 +9.0
HD 150100 12:1 <8.5 - - <12.85 < 1.9 $\times $ 10-8 80.2 $\pm$ 11 +2.0 121 $\pm$ 11 +5.5
HD 176638 10:1 <13.3 - - <13.03 < 6.2 $\times $ 10-8 53.0 $\pm$ 8 -31.0 84 $\pm$ 12 -26.0
HD 188665 13:1 <7.6 - - <12.83 < 1.1 $\times $ 10-8 101.6 $\pm$ 10 -8.5 106 $\pm$ 24 -8.6
HD 201908 7:1 <13.5 - - <13.03 <2.8 $\times $ 10-8 93.0 $\pm$ 8 -19.5 112 $\pm$ 13 -18.5

* = Saturated line blended with CII*1037 Å.

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