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Table 4:

Emission lines of RS Oph on April 2006.
Species $\lambda $ Flux (10-12) RV (km s-1) FWZI
  [Å] (erg s-1 cm-2) narrow blue red (km s-1)
H I            
H$\beta $ 4861 59.1 -21 -38   2500
H$\alpha $ 6562 460 -47     3840
P23 8345 0.6 -19      
P22 8359 1.0 -20      
P21 8374 1.0 -23      
P20 8392 1.3 -20      
P19 8413 2.2 -16      
He I            
  4471 2.6 -19 -205 81 1100
  5875 25.4 -14 -194 155 1950
  6678 9.4 -15 -208   740
  7065 28.1 -17 -196 156 1400
He II            
  4686 26.7 -25 -209 164 1680
  5411 3.4 -21 -208 122 1050
Fe II            
M27 4233 1.9 -20 -186   800
M38 4583 1.7 -20 -272: 77w 650
M42 5169 2.3 -20 -121 123w 580
M49 5234 1.4 -22 -124 134 720
M49 5316 2.4 -18 -195 88w 580
M74 6247 0.8 -22 -141 47 514
M73 7711 1.7 -24 -122 181 717
Raman band 6825 5.1       1470
Forbidden lines            
[O I] 6300 0.6 -15 -94 90 350
[N II] 5754 4.6 -42   81 925
[O III] 5007 1.7 -40 -104   320
Coronal lines            
[Fe XIV] 5303 7.0 -52 -220 163w 900
[A X] 5535($\star$) 7.5 -13 -282 100w 1930
[Fe X] 6375 35.1 -40 -188 166 1500
$\textstyle \parbox{11cm}{
w: very weak line.\\
($\star$ ): blend with Fe {\sc ii}$\lambda$ 5534.9.}$


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