Table D.1
Sample of Mg ii systems with Wr ≥ 1 Å from Lane (2000). The column listings are same as in Table C.1.
| Source | z em | z abs | Wr(Mg iiλ2796) | Wr(Mg iiλ2803) | Wr(Mg iλ2852) | Wr(Fe iiλ2600) | ∫τdv | Mor. | f VLBA | c f | LS |
| (Å) | (Å) | (Å) | (Å) | (km s-1) | (pc) | ||||||
|
|
|||||||||||
| B0109 + 200 | 0.746 | 0.5346 | 2.26 | 1.71 | − | − | < 0.27 | C1 | − | − | − |
| B0229 + 341 | 1.240 | 0.7754 | 1.92 | 2.02 | < 1.13 | − | < 0.43 | R3 | − | − | − |
| B0235 + 164 | 0.940 | 0.5238 | 2.42 | 2.34 | 0.91 | 1.79 | 13.0† | R4 | 0.3–1 | 0.3–1 | < 77 |
| B0420 − 014 | 0.915 | 0.6330 | 1.02 | 0.86 | < 0.36 | − | < 1.59 | C5 | − | − | − |
| B0454 + 039 | 1.343 | 0.8597 | 1.53 | 1.40 | 0.37 | 1.11 | < 0.11 | C | 0.88 | 0.55 | 122 |
| B0805 + 046 | 2.876 | 0.9598 | 1.01 | 0.83 | < 0.60 | 0.24 | < 0.71 | R2 | − | − | − |
| B1218 + 339 | 1.519 | 0.7423 | 1.34 | 1.08 | < 0.70 | 1.00 | < 0.20 | R | 0.07 | 0.07 | < 73 |
| B1327 − 206 | 1.169 | 0.8530 | 2.11 | 1.48 | < 0.40 | 0.76 | < 2.04 | C1 | − | − | − |
| B1354 + 258 | 2.004 | 0.8585 | 1.00 | 0.86 | < 0.10 | < 0.20 | < 1.05 | R | − | − | − |
| B1556 − 245 | 2.815 | 0.7713 | 2.07 | 1.91 | 1.07 | < 0.20 | < 0.68 | C6 | − | − | − |
| B1629 + 120 | 1.795 | 0.5313 | 1.40 | 1.35 | 0.31 | 0.70 | 0.49‡ | C | 0.30 | 0.10 | 71657 |
| ” | 0.9004 | 1.06 | 0.67 | 0.44 | 0.63 | < 0.82 | C | − | − | − | |
| B2212 − 299 | 2.703 | 0.6329 | 1.26 | 1.00 | 0.36 | − | < 2.07 | C1 | − | − | − |
Notes.
21-cm absorption data are from Wolfe et al. (1978).
21-cm absorption data are from Kanekar & Chengalur (2003).
Projected linear size > 2′′ at 5 GHz (Barthel et al. 1988).
Based on Swarup et al. (1984).
Based on the 1.64 GHz image from Murphy et al. (1993).
Unresolved in the 3′′ scale resolution VLA image at 1.4 GHz (Ulvestad et al. 1981).
Compact in the 5 GHz images from Reid et al. (1999) and Barthel et al. (2000).
Based on 2.3 GHz image from Dallacasa et al. (1998); see Saikia et al. (1990) for the subarcsecond scale image at 408 MHz.
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