Table 2: IUE spectra used for the selected symbiotic stars.
Object LWP/LWRa SWPa SWPb
Z And LWP06225 26177 26938
EG And LWP25855 56021 46879
R Aqr LWP21998 31102 40265
T CrB LWP01536 28490  
BF Cyg LWP15253 35843 58386
CH Cyg LWP08631 28011  
CI Cyg LWR10427 18602 50760
AG Dra LWP24400 15656 55373
RW Hya LWR10227 13601  
SY Mus LWR10829 14236 16383
AX Per LWP19332 21443 06807
RX Pup LWR10831 31285 16597
HM Sge LWP12921 40081  
RR Tel LWR16187 20246 18371
KX Tra LWP17871 38742  
PU Vul LWP26780 37190 49265
V1016 Cyg LWP04961 29830 24657
V1329 Cyg LWP13121 24663 05615
HBV475 LWP08277 30853  
a Spectrum with long exposure times used to detect
  weak Fe II fluorescence lines and forbidden lines.
b Spectrum with short exposure times used when allowed
  lines are saturated in longer exposed spectra.

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