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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