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Table 2
Line widths (FWHM) and shifts (uppermost 10 percent) of the strongest broad emission lines.
Emission lines | Width | Shift | Telescope |
[km s-1] | [km s-1] | ||
(1) | (2) | (3) | (4) |
|
|||
O vi λ1038 | 4150 ± 200 | +390 ± 150 | HST |
Lyα | 6300 ± 500 | –860 ± 150 | HST |
Hβ | 4750 ± 200 | 0 | SALT/HET |
Hα | 4010 ± 200 | 0 | SALT |
|
|||
cycA6 λ1082 | 10 200 ± 500 | 0 | HST |
cycB4 λ1136 | 8600 ± 500 | 0 | HST |
cycA5 λ1253 | 12 700 ± 500 | 0 | HST |
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