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Table 1.

FUV absorbers towards the 3C 273.

z Line ID λrest W b N
(Å) (mÅ) (km s−1) log(cm−2)
0.0034 O VI 1031.9 26.6 ± 4.1 ∼28.0 13.353 ± 0.077
0.0073 Lyα 1215.7 28.0 ± 7.0 45.0 ± 14.0 12.740 ± 0.110
0.0076 Lyα 1215.7 43.0 ± 5.0 60.0 ± 10.0 12.940 ± 0.065
0.0076 O VI 1031.9 14.0 ± 4.0 25.0 ± 9.0 13.110 ± 0.160
0.0876 Lyα 1215.7 55.0 ± 1.0 42.0 ± 2.0 13.050 ± 0.020
0.0898 Lyα 1215.7 86.0 ± 4.0 46.0 ± 2.0 13.220 ± 0.070
0.09017 O VI 1031.9 16.0 ± 3.2 22.2 ± 10.8 13.263 ± 0.110
0.09017 O VI 1037.6 14.1 ± 5.0 22.2 ± 10.8 13.263 ± 0.110
0.12005 O VI 1031.9 25.3 ± 3.0 10.0 ± 3.1 13.437 ± 0.058
0.12005 O VI 1037.6 17.8 ± 2.9 10.0 ± 3.1 13.437 ± 0.058

Notes. FUV redshifts of significantly detected BLA’s (b >  40 km s−1) and O VI absorbers in the 3C 273 sight-line (Tilton et al. 2012). The rest-frame line equivalent widths, W, line broadening parameters, b, and HI/O VI column densities, N, are listed with 1σ uncertainties (if available). The emphasized redshifts were considered in this work.

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