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The estimated abundance of O {\\small VI} in the SBs varies from a minimum of (1.09 $\\pm$0.22)$\\times10^{14}$ atoms/cm$^{2}$ in SB N206 to a maximum of (3.71$\\pm$0.23)$\\times10^{14}$ atoms/cm$^{2}$ in SB N70. We find about a 46% excess in the abundance of O {\\small VI} in the SBs compared to the non-SB lines of sight. 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