Table 4: Radial velocities of the IUE emission lines (in units of km s-1).
MJD $\phi$ N V Si IV O IV] N IV] C IV He II O III] N III] Si III] C III]
    1238/42 1394/1403 1400/01/05 1486 1548/50 1640 1660/66 1749/50/52/54 1892 1909
44157 0.718 37/35: 36/42 39/.../44 26 43/42 19 20/20 19/14/8/... 21 15
44401 0.003 47/... 38/41 .../.../... 19 44/40 14 26/14 9/10/13/... 12 10
44719 0.375 27:/... 36:/32: .../.../...  8 39/35 -6 6/7 -9:/10/.../... 11  2
44831 0.506 19/22 26/... .../.../...  4 40/39 -2 11/7 .../ 4/.../... 10 4
45294 0.046 27/20 23/27 .../.../...  2 38/29 2 -4/ 0 .../-8/.../... -5 -1
47786 0.959 .../... .../... .../.../...  1 27/25  3 3/3 .../3/.../5  6  4
48812 0.159 21:/21: .../... .../.../... -3 33/ 34 -17 3/3 .../ 1/.../...  8  0
49486 0.946 15:/24:  9:/27: .../.../...  7 32/29 10 .../2 .../4/.../...  1  9
49520 0.986 21/... 22/... .../.../12 -3 29/22  2 .../-8 .../-3/.../... -4 -2
49676 0.168 33/31 42/35 -1/.../4  2 35/35 -12 1/2 4/3/-1/7  7  3
49827 0.345 16/17 25/19 2/7/13  2 31/27 -23 0/6 6/4/0/1  8  3
49970 0.513 33/29 35/31 14/.../31 17 39/34 -4 18/16 17/21/11/19 25 22

"...'' - too noisy; ":'' - uncertain; for saturated lines the radial velocities (itallic) were obtained by fitting their wings.


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