Table 3: Frequencies detected in the three sets of data for each studied line. The He I 6678 and Mg II 4481 lines are outside the wavelength range of the Musicos spectrograph, and therefore not studied in 2001.
    Frequency (c d-1)
Line Year   $f_{\rm rot}$2-f1f1 2f1
He I 4713 1998 0.480.82 1.01 2.02
  1999 0.500.750.92 1.06 
  2001 0.520.810.941.03 2.02
He I 4921 1998 0.470.750.891.03 2.03
  1999 0.51 0.89? 1.072.06
  2001 0.510.730.93 1.062.06
He I 5876 1998 0.480.750.971.031.072.02
  1999 0.50  1.031.072.06
  2001 0.510.82 1.001.092.03
He I 6678 1998 0.460.820.931.03 2.09
  1999 0.50  1.031.072.06
Mg II 4481 1998 0.480.760.931.04 2.05
  1999 0.500.750.94?1.031.072.06
Si III 4553 1998 0.480.800.921.04 2.07
  1999  0.85 1.031.052.06
  2001 0.470.80.96 1.072.04


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