TABLE I
Emission Lines in Quasars Similar to 0237-233
Emission line data for quasars. Below each wavelength are given, where available,
the characteristics of the line. The symbols have the following meaning.
Br - broad; M - medium strength; S - strong; Wk - weak; VWk - very weak.
For 0029+003, 0046-297, and 2228.6-395, the second line show the equivalent widths.
For 0244-128, 0851+197, and 1448-132, in the second line, the values in decimals
indicate the line to continuum ratios, and the values in Å are the linewidths.
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Quasar V Set 1 2 3 4 5 6 Source
(Mag) (Å) (Å) (Å) (Å) (Å) (Å)
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0237-233 16.63 (a) 3930 4537 4993 5285 6141 Arp et al. (1967)
S M S Wk M
(b) 3919.8 4513.7 Burbidge (1967)
0029+003 18 absent 3994 4507 4991 6160 Shaver et al. (1982)
160 Å 21 Å 73 Å 36 Å
0046-297 19.5 3909 4964 Savage et al. (1985)
200 Å 60 Å
0135-002 19.1 3900 5000 McAlpine and Lewis (1978)
M,Br VWk
0242-410 18.1 3905 3984 4986 5267 6155 Osmer and Smith (1977)
S Wk M Wk Wk
0244-128 17.1 3869 (3989) 4480 4952 5253 6120 Jauncey et al. (1984)
4.46,70Å 0.6 0.5,50Å 2.07,50Å 0.9,15Å 1.0,65Å
0254-671 18.5 3970 4995 Savage and Wright (1981)
0851+197 18 3912 4494 4972 Schmidt (1974)
S,150Å Wk Wk
1225+317 15.87 3930 4950 Ulrich (1976)
S Wk
1246-057 16.73 3976 4983 Osmer and Smith (1977)
S M
1448-232 16.96 (a) 3900 3980 4480 4970 6125 Savage et al. (1976)
2.5,60Å 1.0 0.25 1.0,45Å 0.4,120Å
(b) 3919 4494 4985 Osmer and Smith (1977)
S Wk M
(c) 3911 3985 4515 (4981) Chen et al. (1983, 1984)
1816+475 18.2 3928 4508 4986 Walsh et al. (1979)
2228.6-395 18.3 3895 4479 4971 6094 Savage et al. (1985)
340Å
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